[1] G. O. Abell and B. Margon. A kinematic model for SS433. Nature, 279(5715):701–703, June 1979. doi: 10.1038/279701a0.
[2] A. U. Abeysekara, A. Albert, R. Alfaro, C. Alvarez, J. D. A´lvarez, R. Arceo, J. C. Arteaga- Vel´azquez, D. Avila Rojas, H. A. Ayala Solares, E. Belmont-Moreno, S. Y. BenZvi, C. Bris- bois, K. S. Caballero-Mora, T. Capistr´an, A. Carramin˜ana, S. Casanova, M. Castillo, U. Cotti,J. Cotzomi, S. Coutin˜o de Le´on, C. De Le´on, E. De la Fuente, J. C. D´ıaz-V´elez, S. Dichiara,B. L. Dingus, M. A. DuVernois, R. W. Ellsworth, K. Engel, C. Espinoza, K. Fang, H. Fleis- chhack, N. Fraija, A. Galv´an-G´amez, J. A. Garc´ıa-Gonz´alez, F. Garfias, A. Gonz´alez-Mun˜oz,M. M. Gonz´alez, J. A. Goodman, Z. Hampel-Arias, J. P. Harding, S. Hernandez, J. Hin- ton, B. Hona, F. Hueyotl-Zahuantitla, C. M. Hui, P. Hu¨ntemeyer, A. Iriarte, A. Jardin- Blicq, V. Joshi, S. Kaufmann, P. Kar, G. J. Kunde, R. J. Lauer, W. H. Lee, H. Le´on Var- gas, H. Li, J. T. Linnemann, A. L. Longinotti, G. Luis-Raya, R. L´opez-Coto, K. Malone,S. S. Marinelli, O. Martinez, I. Martinez-Castellanos, J. Mart´ınez-Castro, J. A. Matthews,P. Mirand a-Romagnoli, E. Moreno, M. Mostaf´a, A. Nayerhoda, L. Nellen, M. Newbold,M. U. Nisa, R. Noriega-Papaqui, J. Pretz, E. G. P´erez-P´erez, Z. Ren, C. D. Rho, C. Rivi`ere,D. Rosa-Gonz´alez, M. Rosenberg, E. Ruiz-Velasco, F. Salesa Greus, A. Sandoval, M. Schnei- der, H. Schoorlemmer, M. Seglar Arroyo, G. Sinnis, A. J. Smith, R. W. Springer, P. Surajbali,I. Taboada, O. Tibolla, K. Tollefson, I. Torres, G. Vianello, L. Villasen˜or, T. Weisgarber,F. Werner, S. Westerhoff, J. Wood, T. Yapici, G. Yodh, A. Zepeda, H. Zhang, and H. Zhou. Very-high-energy particle acceleration powered by the jets of the microquasar SS 433. Nature, 562(7725):82–85, Oct. 2018. doi: 10.1038/s41586-018-0565-5.
[3] F. Aharonian, A. G. Akhperjanian, A. R. Bazer-Bachi, M. Beilicke, W. Benbow, D. Berge,K. Bernl¨ohr, C. Boisson, O. Bolz, V. Borrel, I. Braun, F. Breitling, A. M. Brown, P. M. Chad- wick, L. M. Chounet, R. Cornils, L. Costamante, B. Degrange, H. J. Dickinson, A. Djannati- Ata¨ı, L. O’C. Drury, G. Dubus, D. Emmanoulopoulos, P. Espigat, F. Feinstein, G. Fontaine,Y. Fuchs, S. Funk, Y. A. Gallant, B. Giebels, J. F. Glicenstein, P. Goret, C. Hadjichristidis,D. Hauser, M. Hauser, G. Heinzelmann, G. Henri, G. Hermann, J. A. Hinton, W. Hofmann,M. Holleran, D. Horns, A. Jacholkowska, O. C. de Jager, B. Kh´elifi, S. Klages, N. Komin,A. Konopelko, I. J. Latham, R. Le Gallou, A. Lemi`ere, M. Lemoine-Goumard, T. Lohse,J. M. Martin, O. Martineau-Huynh, A. Marcowith, C. Masterson, T. J. L. McComb, M. de Naurois, D. Nedbal, S. J. Nolan, A. Noutsos, K. J. Orford, J. L. Osborne, M. Ouchrif,M. Panter, G. Pelletier, S. Pita, G. Pu¨hlhofer, M. Punch, B. C. Raubenheimer, M. Raue,S. M. Rayner, A. Reimer, O. Reimer, J. Ripken, L. Rob, L. Rolland, G. Rowell, V. Sahakian,L. Saug´e, S. Schlenker, R. Schlickeiser, C. Schuster, U. Schwanke, M. Siewert, H. Sol, D. Span- gler, R. Steenkamp, C. Stegmann, G. Superina, J. P. Tavernet, R. Terrier, C. G. Th´eoret,M. Tluczykont, C. van Eldik, G. Vasileiadis, C. Venter, P. Vincent, H. J. V¨olk, and S. J. Wag- ner. A detailed spectral and morphological study of the gamma-ray supernova remnant RX J1713.7-3946 with HESS. A&A, 449(1):223–242, Apr. 2006. doi: 10.1051/0004-6361:20054279.
[4] C. S. Anderson, B. M. Gaensler, and I. J. Feain. A Study of Broadband Faraday Rotation and Polarization Behavior over 1.3–10 GHz in 36 Discrete Radio Sources. ApJ, 825(1):59, July 2016. doi: 10.3847/0004-637X/825/1/59.
[5] Y. Asahina, T. Ogawa, T. Kawashima, N. Furukawa, R. Enokiya, H. Yamamoto, Y. Fukui, and R. Matsumoto. Magnetohydrodynamic Simulations of a Jet Drilling an H I Cloud: Shock Induced Formation of Molecular Clouds and Jet Breakup. ApJ, 789(1):79, July 2014. doi: 10.1088/0004-637X/789/1/79.
[6] J. Baba, Y. Asaki, J. Makino, M. Miyoshi, T. R. Saitoh, and K. Wada. The Origin of Large Peculiar Motions of Star-Forming Regions and Spiral Structures of Our Galaxy. ApJ, 706(1): 471–481, Nov. 2009. doi: 10.1088/0004-637X/706/1/471.
[7] R. Beck and M. Krause. Revised equipartition and minimum energy formula for magnetic field strength estimates from radio synchrotron observations. Astronomische Nachrichten, 326 (6):414–427, July 2005. doi: 10.1002/asna.200510366.
[8] A. R. Bell. The acceleration of cosmic rays in shock fronts - I. MNRAS, 182:147–156, Jan. 1978a. doi: 10.1093/mnras/182.2.147.
[9] A. R. Bell. The acceleration of cosmic rays in shock fronts - II. MNRAS, 182:443–455, Feb. 1978b. doi: 10.1093/mnras/182.3.443.
[10] R. D. Blandford. On the mediation of a shock front by Fermi-accelerated cosmic rays. ApJ, 238:410–416, May 1980. doi: 10.1086/157998.
[11] K. M. Blundell and M. G. Bowler. Symmetry in the Changing Jets of SS 433 and Its True Distance from Us. ApJL, 616(2):L159–L162, Dec. 2004. doi: 10.1086/426542.
[12] K. M. Blundell, R. Laing, S. Lee, and A. Richards. SS433’s Jet Trace from ALMA Imaging and Global Jet Watch Spectroscopy: Evidence for Post-launch Particle Acceleration. ApJL, 867(2):L25, Nov. 2018. doi: 10.3847/2041-8213/aae890.
[13] A. D. Bolatto, M. Wolfire, and A. K. Leroy. The CO-to-H2 Conversion Factor. ARA&A, 51(1):207–268, Aug. 2013. doi: 10.1146/annurev-astro-082812-140944.
[14] P. Bordas, R. Yang, E. Kafexhiu, and F. Aharonian. Detection of Persistent Gamma-Ray Emission Toward SS433/W50. ApJL, 807(1):L8, July 2015. doi: 10.1088/2041-8205/807/1/L8.
[15] J. Brand and L. Blitz. The velocity field of the outer galaxy. A&A, 275:67–90, Aug. 1993.
[16] R. Braun, A. Bonaldi, T. Bourke, E. Keane, and J. Wagg. Anticipated Performance of the Square Kilometre Array – Phase 1 (SKA1). arXiv e-prints, art. arXiv:1912.12699, Dec. 2019.
[17] M. A. Brentjens and A. G. de Bruyn. Faraday rotation measure synthesis. A&A, 441(3): 1217–1228, Oct. 2005. doi: 10.1051/0004-6361:20052990.
[18] W. Brinkmann, B. Aschenbach, and N. Kawai. ROSAT observations of the W 50/SS 433 system. A&A, 312:306–316, Aug. 1996.
[19] W. Brinkmann, G. W. Pratt, S. Rohr, N. Kawai, and V. Burwitz. XMM-Newton obser- vations of the eastern jet of SS 433. A&A, 463(2):611–619, Feb. 2007. doi: 10.1051/0004- 6361:20065570.
[20] J. W. Broderick, R. P. Fender, J. C. A. Miller-Jones, S. A. Trushkin, A. J. Stewart, G. E. Anderson, T. D. Staley, K. M. Blundell, M. Pietka, S. Markoff, A. Rowlinson, J. D. Swinbank,A. J. van der Horst, M. E. Bell, R. P. Breton, D. Carbone, S. Corbel, J. Eisl¨offel, H. Falcke,J. M. Grießmeier, J. W. T. Hessels, V. I. Kondratiev, C. J. Law, G. J. Molenaar, M. Serylak,B. W. Stappers, J. van Leeuwen, R. A. M. J. Wijers, R. Wijnands, M. W. Wise, and P. Zarka. LOFAR 150-MHz observations of SS 433 and W 50. MNRAS, 475(4):5360–5377, Apr. 2018.doi: 10.1093/mnras/sty081.
[21] J. I. Castor. Spectral line formation in Wolf-Rayet envelopes. MNRAS, 149:111, Jan. 1970. doi: 10.1093/mnras/149.2.111.
[22] L. Ciotti and A. D’Ercole. SNR expansion in a pre-existent cavity. A&A, 215:347–359, May 1989.
[23] A. J. Cooper, D. Gaggero, S. Markoff, and S. Zhang. High-energy cosmic ray production in X-ray binary jets. MNRAS, 493(3):3212–3222, Feb. 2020. doi: 10.1093/mnras/staa373.
[24] W. Dehnen and J. Binney. Mass models of the Milky Way. MNRAS, 294(3):429–438, Mar. 1998. doi: 10.1046/j.1365-8711.1998.01282.x.
[25] J. M. Dickey and F. J. Lockman. H I in the galaxy. ARA&A, 28:215–261, Jan. 1990. doi: 10.1146/annurev.aa.28.090190.001243.
[26] S. D’Odorico, T. Oosterloo, T. Zwitter, and M. Calvani. Evidence that the compact object in SS433 is a neutron star and not a black hole. Nature, 353(6342):329–331, Sept. 1991. doi: 10.1038/353329a0.
[27] A. J. B. Downes, T. Pauls, and C. J. Salter. Further radio observations of W 50 : total intensity and linear polarisation measurements at 1.7 and 2.7 GHz. A&A, 103:277–287, Nov. 1981a.
[28] A. J. B. Downes, C. J. Salter, and T. Pauls. Radio observations at 1720 MHz of the area L equals 38.5 to 43.5 deg and B equals -5 to 5 deg - The region surrounding W 50. A&A, 97 (2):296–301, Apr. 1981b.
[29] A. J. B. Downes, T. Pauls, and C. J. Salter. The supernova remnant W 50 at 5 GHz.MNRAS, 218:393–407, Feb. 1986. doi: 10.1093/mnras/218.3.393.
[30] J. F. Drake, M. Opher, M. Swisdak, and J. N. Chamoun. A Magnetic Reconnection Mech- anism for the Generation of Anomalous Cosmic Rays. ApJ, 709(2):963–974, Feb. 2010. doi: 10.1088/0004-637X/709/2/963.
[31] L. O. Drury. REVIEW ARTICLE: An introduction to the theory of diffusive shock ac- celeration of energetic particles in tenuous plasmas. Reports on Progress in Physics, 46(8): 973–1027, Aug. 1983. doi: 10.1088/0034-4885/46/8/002.
[32] G. M. Dubner, M. Holdaway, W. M. Goss, and I. F. Mirabel. A High-Resolution Radio Study of the W50-SS 433 System and the Surrounding Medium. AJ, 116(4):1842–1855, Oct. 1998. doi: 10.1086/300537.
[33] S. S. Eikenberry, P. B. Cameron, B. W. Fierce, D. M. Kull, D. H. Dror, J. R. Houck, and B. Margon. Twenty Years of Timing SS 433. ApJ, 561(2):1027–1033, Nov. 2001. doi: 10.1086/323380.
[34] R. Elston and S. Baum. High-Resolution Radio Observations of W50, the Remnant Asso- ciated with SS 433. AJ, 94:1633, Dec. 1987. doi: 10.1086/114594.
[35] K. Fang, E. Charles, and R. D. Blandford. GeV-TeV Counterparts of SS 433/W50 from Fermi-LAT and HAWC Observations. ApJL, 889(1):L5, Jan. 2020. doi: 10.3847/2041- 8213/ab62b8.
[36] J. S. Farnes, B. M. Gaensler, C. Purcell, X. H. Sun, M. Haverkorn, E. Lenc, S. P. O’Sullivan, and T. Akahori. Interacting large-scale magnetic fields and ionized gas in the W50/SS433 system. MNRAS, 467(4):4777–4801, June 2017. doi: 10.1093/mnras/stx338.
[37] Y. Fukui, H. Sano, J. Sato, K. Torii, H. Horachi, T. Hayakawa, N. M. McClure-Griffiths,G. Rowell, T. Inoue, S. Inutsuka, A. Kawamura, H. Yamamoto, T. Okuda, N. Mizuno, T. On- ishi, A. Mizuno, and H. Ogawa. A Detailed Study of the Molecular and Atomic Gas toward the γ-Ray Supernova Remnant RX J1713.7-3946: Spatial TeV γ-Ray and Interstellar Medium Gas Correspondence. ApJ, 746(1):82, Feb. 2012. doi: 10.1088/0004-637X/746/1/82.
[38] Y. Fukui, K. Torii, T. Onishi, H. Yamamoto, R. Okamoto, T. Hayakawa, K. Tachihara, andH. Sano. Optically Thick H I Dominant in the Local Interstellar Medium: An Alternative Interpretation to “Dark Gas”. ApJ, 798(1):6, Jan. 2015. doi: 10.1088/0004-637X/798/1/6.
[39] Y. Fukui, H. Sano, J. Sato, R. Okamoto, T. Fukuda, S. Yoshiike, K. Hayashi, K. Torii,T. Hayakawa, G. Rowell, M. D. Filipovi´c, N. Maxted, N. M. McClure-Griffiths, A. Kawamura,H. Yamamoto, T. Okuda, N. Mizuno, K. Tachihara, T. Onishi, A. Mizuno, and H. Ogawa. A Detailed Study of the Interstellar Protons toward the TeV γ-Ray SNR RX J0852.0-4622 (G266.2-1.2, Vela Jr.): The Third Case of the γ-Ray and ISM Spatial Correspondence. ApJ, 850(1):71, Nov. 2017. doi: 10.3847/1538-4357/aa9219.
[40] Gaia Collaboration, A. G. A. Brown, A. Vallenari, T. Prusti, J. H. J. de Bruijne, C. Babu- siaux, C. A. L. Bailer-Jones, M. Biermann, D. W. Evans, L. Eyer, F. Jansen, C. Jordi, S. A. Klioner, U. Lammers, L. Lindegren, X. Luri, F. Mignard, C. Panem, D. Pourbaix, S. Randich,P. Sartoretti, H. I. Siddiqui, C. Soubiran, F. van Leeuwen, N. A. Walton, F. Arenou, U. Bas- tian, M. Cropper, R. Drimmel, D. Katz, M. G. Lattanzi, J. Bakker, C. Cacciari, J. Castan˜eda,L. Chaoul, N. Cheek, F. De Angeli, C. Fabricius, R. Guerra, B. Holl, E. Masana, R. Messineo,N. Mowlavi, K. Nienartowicz, P. Panuzzo, J. Portell, M. Riello, G. M. Seabroke, P. Tanga,F. Th´evenin, G. Gracia-Abril, G. Comoretto, M. Garcia-Reinaldos, D. Teyssier, M. Altmann,R. Andrae, M. Audard, I. Bellas-Velidis, K. Benson, J. Berthier, R. Blomme, P. Burgess,G. Busso, B. Carry, A. Cellino, G. Clementini, M. Clotet, O. Creevey, M. Davidson, J. De Ridder, L. Delchambre, A. Dell’Oro, C. Ducourant, J. Fern´andez-Hern´andez, M. Fouesneau,Y. Fr´emat, L. Galluccio, M. Garc´ıa-Torres, J. Gonz´alez-Nu´n˜ez, J. J. Gonz´alez-Vidal, E. Gos- set, L. P. Guy, J. L. Halbwachs, N. C. Hambly, D. L. Harrison, J. Hern´andez, D. Hestroffer,S. T. Hodgkin, A. Hutton, G. Jasniewicz, A. Jean-Antoine-Piccolo, S. Jordan, A. J. Korn,A. Krone-Martins, A. C. Lanzafame, T. Lebzelter, W. L¨offler, M. Manteiga, P. M. Mar- rese, J. M. Mart´ın-Fleitas, A. Moitinho, A. Mora, K. Muinonen, J. Osinde, E. Pancino,T. Pauwels, J. M. Petit, A. Recio-Blanco, P. J. Richards, L. Rimoldini, A. C. Robin, L. M. Sarro, C. Siopis, M. Smith, A. Sozzetti, M. Su¨veges, J. Torra, W. van Reeven, U. Abbas,A. Abreu Aramburu, S. Accart, C. Aerts, G. Altavilla, M. A. A´lvarez, R. Alvarez, J. Alves,R. I. Anderson, A. H. Andrei, E. Anglada Varela, E. Antiche, T. Antoja, B. Arcay, T. L. Astraatmadja, N. Bach, S. G. Baker, L. Balaguer-Nu´n˜ez, P. Balm, C. Barache, C. Barata,D. Barbato, F. Barblan, P. S. Barklem, D. Barrado, M. Barros, M. A. Barstow, S. Bartholom´e Mun˜oz, J. L. Bassilana, U. Becciani, M. Bellazzini, A. Berihuete, S. Bertone, L. Bianchi, O. Bi- enaym´e, S. Blanco-Cuaresma, T. Boch, C. Boeche, A. Bombrun, R. Borrachero, D. Bossini,S. Bouquillon, G. Bourda, A. Bragaglia, L. Bramante, M. A. Breddels, A. Bressan, N. Brouil- let, T. Bru¨semeister, E. Brugaletta, B. Bucciarelli, A. Burlacu, D. Busonero, A. G. Butke- vich, R. Buzzi, E. Caffau, R. Cancelliere, G. Cannizzaro, T. Cantat-Gaudin, R. Carballo,T. Carlucci, J. M. Carrasco, L. Casamiquela, M. Castellani, A. Castro-Ginard, P. Charlot,L. Chemin, A. Chiavassa, G. Cocozza, G. Costigan, S. Cowell, F. Crifo, M. Crosta, C. Crow- ley, J. Cuypers, C. Dafonte, Y. Damerdji, A. Dapergolas, P. David, M. David, P. de Laverny,F. De Luise, R. De March, D. de Martino, R. de Souza, A. de Torres, J. Debosscher, E. del Pozo, M. Delbo, A. Delgado, H. E. Delgado, P. Di Matteo, S. Diakite, C. Diener, E. Distefano,C. Dolding, P. Drazinos, J. Dur´an, B. Edvardsson, H. Enke, K. Eriksson, P. Esquej, G. Ey- nard Bontemps, C. Fabre, M. Fabrizio, S. Faigler, A. J. Falc˜ao, M. Farr`as Casas, L. Federici,G. Fedorets, P. Fernique, F. Figueras, F. Filippi, K. Findeisen, A. Fonti, E. Fraile, M. Fraser,B. Fr´ezouls, M. Gai, S. Galleti, D. Garabato, F. Garc´ıa-Sedano, A. Garofalo, N. Garralda,A. Gavel, P. Gavras, J. Gerssen, R. Geyer, P. Giacobbe, G. Gilmore, S. Girona, G. Giuf- frida, F. Glass, M. Gomes, M. Granvik, A. Gueguen, A. Guerrier, J. Guiraud, R. Guti´errez- S´anchez, R. Haigron, D. Hatzidimitriou, M. Hauser, M. Haywood, U. Heiter, A. Helmi, J. Heu,T. Hilger, D. Hobbs, W. Hofmann, G. Holland, H. E. Huckle, A. Hypki, V. Icardi, K. Janßen,G. Jevardat de Fombelle, P. G. Jonker, A´. L. Juh´asz, F. Julbe, A. Karampelas, A. Kewley,J. Klar, A. Kochoska, R. Kohley, K. Kolenberg, M. Kontizas, E. Kontizas, S. E. Koposov,G. Kordopatis, Z. Kostrzewa-Rutkowska, P. Koubsky, S. Lambert, A. F. Lanza, Y. Lasne, J. B. Lavigne, Y. Le Fustec, C. Le Poncin-Lafitte, Y. Lebreton, S. Leccia, N. Leclerc, I. Lecoeur- Taibi, H. Lenhardt, F. Leroux, S. Liao, E. Licata, H. E. P. Lindstrøm, T. A. Lister, E. Livanou,A. Lobel, M. L´opez, S. Managau, R. G. Mann, G. Mantelet, O. Marchal, J. M. Marchant,M. Marconi, S. Marinoni, G. Marschalk´o, D. J. Marshall, M. Martino, G. Marton, N. Mary,D. Massari, G. Matijeviˇc, T. Mazeh, P. J. McMillan, S. Messina, D. Michalik, N. R. Millar,D. Molina, R. Molinaro, L. Moln´ar, P. Montegriffo, R. Mor, R. Morbidelli, T. Morel, D. Morris,A. F. Mulone, T. Muraveva, I. Musella, G. Nelemans, L. Nicastro, L. Noval, W. O’Mullane,C. Ord´enovic, D. Ord´on˜ez-Blanco, P. Osborne, C. Pagani, I. Pagano, F. Pailler, H. Palacin,L. Palaversa, A. Panahi, M. Pawlak, A. M. Piersimoni, F. X. Pineau, E. Plachy, G. Plum,E. Poggio, E. Poujoulet, A. Prˇsa, L. Pulone, E. Racero, S. Ragaini, N. Rambaux, M. Ramos- Lerate, S. Regibo, C. Reyl´e, F. Riclet, V. Ripepi, A. Riva, A. Rivard, G. Rixon, T. Roegiers,M. Roelens, M. Romero-G´omez, N. Rowell, F. Royer, L. Ruiz-Dern, G. Sadowski, T. Sagrist`a Sell´es, J. Sahlmann, J. Salgado, E. Salguero, N. Sanna, T. Santana-Ros, M. Sarasso, H. Savi- etto, M. Schultheis, E. Sciacca, M. Segol, J. C. Segovia, D. S´egransan, I. C. Shih, L. Siltala,A. F. Silva, R. L. Smart, K. W. Smith, E. Solano, F. Solitro, R. Sordo, S. Soria Nieto,J. Souchay, A. Spagna, F. Spoto, U. Stampa, I. A. Steele, H. Steidelmu¨ller, C. A. Stephen- son, H. Stoev, F. F. Suess, J. Surdej, L. Szabados, E. Szegedi-Elek, D. Tapiador, F. Taris,G. Tauran, M. B. Taylor, R. Teixeira, D. Terrett, P. Teyssandier, W. Thuillot, A. Titarenko,F. Torra Clotet, C. Turon, A. Ulla, E. Utrilla, S. Uzzi, M. Vaillant, G. Valentini, V. Valette,A. van Elteren, E. Van Hemelryck, M. van Leeuwen, M. Vaschetto, A. Vecchiato, J. Veljanoski,Y. Viala, D. Vicente, S. Vogt, C. von Essen, H. Voss, V. Votruba, S. Voutsinas, G. Walmsley,M. Weiler, O. Wertz, T. Wevers, L- . Wyrzykowski, A. Yoldas, M. Zˇerjal, H. Ziaeepour, J. Zorec,S. Zschocke, S. Zucker, C. Zurbach, and T. Zwitter. Gaia Data Release 2. Summary of the contents and survey properties. A&A, 616:A1, Aug. 2018. doi: 10.1051/0004-6361/201833051.
[41] Gaia Collaboration, A. G. A. Brown, A. Vallenari, T. Prusti, J. H. J. de Bruijne, C. Babu- siaux, and M. Biermann. Gaia Early Data Release 3: Summary of the contents and survey properties. arXiv e-prints, art. arXiv:2012.01533, Dec. 2020.
[42] V. Gaibler, M. Krause, and M. Camenzind. Very light magnetized jets on large scales - I. Evolution and magnetic fields. MNRAS, 400(4):1785–1802, Dec. 2009. doi: 10.1111/j.1365- 2966.2009.15625.x.
[43] B. J. Geldzahler, T. Pauls, and C. J. Salter. Continuum observations of the SNR W50 and G 74.9+1.2 at 2695 MHz. A&A, 84:237–244, Apr. 1980.
[44] V. L. Ginzburg and S. I. Syrovatskii. The Origin of Cosmic Rays. 1964.
[45] P. Goldreich and J. Kwan. Molecular Clouds. ApJ, 189:441–454, May 1974. doi: 10.1086/152821.
[46] P. T. Goodall, F. Alouani-Bibi, and K. M. Blundell. When microquasar jets and supernova collide: hydrodynamically simulating the SS 433-W 50 interaction. MNRAS, 414(4):2838– 2859, July 2011a. doi: 10.1111/j.1365-2966.2011.18388.x.
[47] P. T. Goodall, K. M. Blundell, and S. J. Bell Burnell. Probing the history of SS 433’sjet kinematics via decade-resolution radio observations of W 50. MNRAS, 414(4):2828–2837, July 2011b. doi: 10.1111/j.1365-2966.2011.18809.x.
[48] V. P. Goranskii, V. F. Esipov, and A. M. Cherepashchuk. Optical variability of SS 433 in 1978-1996. Astronomy Reports, 42(2):209–228, Mar. 1998.
[49] T. C. Hillwig and D. R. Gies. Spectroscopic Observations of the Mass Donor Star in SS433. ApJL, 676(1):L37, Mar. 2008. doi: 10.1086/587140.
[50] T. C. Hillwig, D. R. Gies, W. Huang, M. V. McSwain, M. A. Stark, A. van der Meer, andL. Kaper. Identification of the Mass Donor Star’s Spectrum in SS 433. ApJ, 615(1):422–431, Nov. 2004. doi: 10.1086/423927.
[51] R. M. Hjellming and K. J. Johnston. An analysis of the proper motions of SS 433 radio jets. ApJL, 246:L141–L145, June 1981. doi: 10.1086/183571.
[52] E. J. Hodges-Kluck and C. S. Reynolds. Hydrodynamic Models of Radio Galaxy Morphology: Winged and X-shaped Sources. ApJ, 733(1):58, May 2011. doi: 10.1088/0004-637X/733/1/58.
[53] M. Hoshino and N. Shimada. Nonthermal Electrons at High Mach Number Shocks: Electron Shock Surfing Acceleration. ApJ, 572(2):880–887, June 2002. doi: 10.1086/340454.
[54] S. Ideguchi, K. Takahashi, T. Akahori, K. Kumazaki, and D. Ryu. Fisher analysis on wide- band polarimetry for probing the intergalactic magnetic field. PASJ, 66(1):5, Feb. 2014. doi: 10.1093/pasj/pst007.
[55] R. M. Jeffrey, K. M. Blundell, S. A. Trushkin, and A. J. Mioduszewski. Fast launch speeds in radio flares, from a new determination of the intrinsic motions of SS 433’s jet bolides. MNRAS, 461(1):312–320, Sept. 2016. doi: 10.1093/mnras/stw1322.
[56] F. J. Kerr. Radio-Line Emission and Absorption by the Interstellar Gas, page 575. 1968.
[57] S. S. Kimura, K. Murase, and P. M´esz´aros. Deciphering the Origin of the GeV ─ TeV Gamma-Ray Emission from SS 433. ApJ, 904(2):188, Dec. 2020. doi: 10.3847/1538- 4357/abbe00.
[58] A. Konigl. W 50 - a stellar-wind bubble in a three-phase intestellar medium ? MNRAS, 205:471–485, Nov. 1983. doi: 10.1093/mnras/205.2.471.
[59] K. Kubota, Y. Ueda, N. Kawai, T. Kotani, M. Namiki, K. Kinugasa, S. Ozaki, T. Iijima,S. Fabrika, T. Yuasa, S. Yamada, and K. Makishima. Suzaku X-Ray and Optical Spectroscopic Observations of SS 433 in the 2006 April Multiwavelength Campaign. PASJ, 62:323, Apr. 2010. doi: 10.1093/pasj/62.2.323.
[60] P. O. Lagage and C. J. Cesarsky. The maximum energy of cosmic rays accelerated by supernova shocks. A&A, 125:249–257, Sept. 1983.
[61] J. Li, D. F. Torres, R.-Y. Liu, M. Kerr, E. de On˜a Wilhelmi, and Y. Su. Gamma-ray heartbeat powered by the microquasar SS 433. Nature Astronomy, 4:1177–1184, Jan. 2020. doi: 10.1038/s41550-020-1164-6.
[62] Q.-C. Liu, Y. Chen, P. Zhou, X. Zhang, and B. Jiang. A Small-Scale Investigation of Molecular Emission toward the Tip of the Western Lobe of W50/SS433. arXiv e-prints, art. arXiv:2002.09829, Feb. 2020.
[63] F. J. Lockman, K. M. Blundell, and W. M. Goss. The distance to SS433/W50 and its inter- action with the interstellar medium. MNRAS, 381(3):881–893, Nov. 2007. doi: 10.1111/j.1365- 2966.2007.12170.x.
[64] B. Margon. Observations of SS 433. ARA&A, 22:507–536, Jan. 1984. doi: 10.1146/an- nurev.aa.22.090184.002451.
[65] B. Margon, H. C. Ford, S. A. Grandi, and R. P. S. Stone. Enormous periodic Doppler shifts in SS433. ApJL, 233:L63–L68, Oct. 1979. doi: 10.1086/183077.
[66] A. J. Mioduszewski, V. Dhawan, and M. P. Rupen. Recent Results of VLBA Imaging of X-Ray Binaries: the Newest and Oldest Microquasars. In J. Romney and M. Reid, editors, Future Directions in High Resolution Astronomy, volume 340 of Astronomical Society of the Pacific Conference Series, page 281, Dec. 2005.
[67] I. F. Mirabel and L. F. Rodr´ıguez. Microquasars in our Galaxy. Nature, 392(6677):673–676, Apr. 1998. doi: 10.1038/33603.
[68] R. Monceau-Baroux, O. Porth, Z. Meliani, and R. Keppens. The SS433 jet from subparsec to parsec scales. A&A, 574:A143, Feb. 2015. doi: 10.1051/0004-6361/201425015.
[69] C. A. Norman, D. B. Melrose, and A. Achterberg. The Origin of Cosmic Rays above 1018.5 eV. ApJ, 454:60, Nov. 1995. doi: 10.1086/176465.
[70] T. Ohmura, K. Ono, H. Sakemi, Y. Tashima, R. Omae, and M. Machida. Continuous jets and backflow models for the formation of w50/ss433 in magnetohydrodynamical simulations. ApJ, 2021.
[71] S. P. O’Sullivan, S. Brown, T. Robishaw, D. H. F. M. Schnitzeler, N. M. McClure-Griffiths,I. J. Feain, A. R. Taylor, B. M. Gaensler, T. L. Land ecker, L. Harvey-Smith, and E. Carretti.Complex Faraday depth structure of active galactic nuclei as revealed by broad-band radio polarimetry. MNRAS, 421(4):3300–3315, Apr. 2012. doi: 10.1111/j.1365-2966.2012.20554.x.
[72] T. Ozawa, H. Nakanishi, T. Akahori, K. Anraku, M. Takizawa, I. Takahashi, S. Onodera,Y. Tsuda, and Y. Sofue. JVLA S- and X-band polarimetry of the merging cluster Abell 2256.PASJ, 67(6):110, Dec. 2015. doi: 10.1093/pasj/psv082.
[73] A. A. Panferov. Jets of SS 433 on scales of dozens of parsecs. A&A, 599:A77, Mar. 2017. doi: 10.1051/0004-6361/201629256.
[74] Z. Paragi, R. C. Vermeulen, I. Fejes, R. T. Schilizzi, R. E. Spencer, and A. M. Stirling. The inner radio jet region and the complex environment of SS433. A&A, 348:910–916, Aug. 1999.
[75] J. E. G. Peek, C. Heiles, K. A. Douglas, M.-Y. Lee, J. Grcevich, S. Stanimirovi´c, M. E. Put- man, E. J. Korpela, S. J. Gibson, A. Begum, D. Saul, T. Robishaw, and M. Krˇco. The GALFA- HI Survey: Data Release 1. ApJS, 194(2):20, June 2011. doi: 10.1088/0067-0049/194/2/20.
[76] F. G. Ram´on-Fox and I. A. Bonnell. Streaming motions and kinematic distances to molecular clouds. MNRAS, 474(2):2028–2038, Feb. 2018. doi: 10.1093/mnras/stx2866.
[77] D. H. Roberts, J. P. Cohen, J. Lu, L. Saripalli, and R. Subrahmanyan. The Abundance of X-shaped Radio Sources. I. VLA Survey of 52 Sources with Off-axis Distortions. ApJS, 220 (1):7, Sept. 2015. doi: 10.1088/0067-0049/220/1/7.
[78] P. Rossi, G. Bodo, A. Capetti, and S. Massaglia. 3D relativistic MHD numerical simulations of X-shaped radio sources. A&A, 606:A57, Oct. 2017. doi: 10.1051/0004-6361/201730594.
[79] M. Rozyczka, G. Tenorio-Tagle, J. Franco, and P. Bodenheimer. On the evolution of supernova remnants. III. Off-centred supernova explosions in pre-existing wind-driven bubbles. MNRAS, 261:674–680, Apr. 1993. doi: 10.1093/mnras/261.3.674.
[80] S. Safi-Harb and H. O¨ gelman. ROSAT and ASCA Observations of W50 Associated with the Peculiar Source SS 433. ApJ, 483(2):868–881, July 1997. doi: 10.1086/304274.
[81] S. Safi-Harb and R. Petre. Rossi X-Ray Timing Explorer Observations of the Eastern Lobe of W50 Associated with SS 433. ApJ, 512(2):784–792, Feb. 1999. doi: 10.1086/306803.
[82] H. Sakemi, M. Machida, T. Akahori, H. Nakanishi, H. Akamatsu, K. Kurahara, andJ. Farnes. Magnetic field analysis of the bow and terminal shock of the SS 433 jet. PASJ, 70 (2):27, Mar. 2018. doi: 10.1093/pasj/psy003.
[83] H. Sano, E. M. Reynoso, I. Mitsuishi, K. Nakamura, N. Furukawa, K. Mruganka, T. Fukuda,S. Yoshiike, A. Nishimura, A. Ohama, K. Torii, T. Kuwahara, T. Okuda, H. Yamamoto,K. Tachihara, and Y. Fukui. Interstellar gas and X-rays toward the Young supernova remnant RCW 86; pursuit of the origin of the thermal and non-thermal X-ray. Journal of High Energy Astrophysics, 15:1–18, Sept. 2017. doi: 10.1016/j.jheap.2017.04.002.
[84] H. Sano, H. Matsumura, Y. Yamane, P. Maggi, K. Fujii, K. Tsuge, K. Tokuda, R. Z. E. Alsaberi, M. D. Filipovi´c, N. Maxted, G. Rowell, H. Uchida, T. Tanaka, K. Muraoka,T. Takekoshi, T. Onishi, A. Kawamura, T. Minamidani, N. Mizuno, H. Yamamoto, K. Tachi- hara, T. Inoue, S. Inutsuka, F. Voisin, N. F. H. Tothill, M. Sasaki, N. M. McClure-Griffiths, and Y. Fukui. Discovery of Shocked Molecular Clouds Associated with the Shell-type Super- nova Remnant RX J0046.5-7308 in the Small Magellanic Cloud. ApJ, 881(1):85, Aug. 2019. doi: 10.3847/1538-4357/ab2ade.
[85] D. Schnitzeler, B. Gaensler, L. Staveley-Smith, E. Carretti, M. Haverkorn, M. Kesteven,S. Poppi, J. Stevens, and G. Bernardi. Unveiling the Galactic Magnetic Field in the Southern Sky. ATNF Proposal, Oct. 2011.
[86] C. B. Stephenson and N. Sanduleak. New H-alpha emission stars in the Milky Way. ApJS, 33:459–469, Apr. 1977. doi: 10.1086/190437.
[87] Y. Su, X. Zhou, J. Yang, Y. Chen, X. Chen, and S. Zhang. The Large-scale Interstel- lar Medium of SS 433/W50 Revisited. ApJ, 863(1):103, Aug. 2018. doi: 10.3847/1538- 4357/aad04e.
[88] T. Sudoh, Y. Inoue, and D. Khangulyan. Multiwavelength Emission from Galactic Jets: The Case of the Microquasar SS433. ApJ, 889(2):146, Feb. 2020. doi: 10.3847/1538-4357/ab6442.
[89] X.-N. Sun, R.-Z. Yang, B. Liu, S.-Q. Xi, and X.-Y. Wang. Tentative evidence of spatially extended GeV emission from SS433/W50. A&A, 626:A113, June 2019. doi: 10.1051/0004- 6361/201935621.
[90] G. Tenorio-Tagle, M. Rozyczka, J. Franco, and P. Bodenheimer. On the evolution of supernova remnants - II. Two-dimensional calculationsof explosions inside pre-existing wind- driven bubbles. MNRAS, 251:318, July 1991. doi: 10.1093/mnras/251.2.318.
[91] F. F. S. van der Tak, J. H. Black, F. L. Sch¨oier, D. J. Jansen, and E. F. van Dishoeck. A computer program for fast non-LTE analysis of interstellar line spectra. With diagnos- tic plots to interpret observed line intensity ratios. A&A, 468(2):627–635, June 2007. doi: 10.1051/0004-6361:20066820.
[92] M. Vietri. The Acceleration of Ultra–High-Energy Cosmic Rays in Gamma-Ray Bursts.ApJ, 453:883, Nov. 1995. doi: 10.1086/176448.
[93] M. G. Watson, R. Willingale, J. E. Grindlay, and F. D. Seward. The X-ray lobes of SS 433.ApJ, 273:688–696, Oct. 1983. doi: 10.1086/161403.
[94] G. Westerhout. A survey of the continuous radiation from the Galactic System at a frequency of 1390 Mc/s. Bulletin of the Astronomical Institutes of the Netherlands, 14:215, Dec. 1958.
[95] H. Yamamoto, S. Ito, S. Ishigami, M. Fujishita, T. Kawase, A. Kawamura, N. Mizuno,T. Onishi, A. Mizuno, N. M. McClure-Griffiths, and Y. Fukui. Aligned Molecular Clouds towards SS 433 and L = 348.5: Possible Evidence for a Galactic “Vapor Trail” Created by a Relativistic Jet. PASJ, 60:715, Aug. 2008. doi: 10.1093/pasj/60.4.715.
[96] L. Zaninetti. Classical and relativistic flux of energy conservation in astrophysical jets.arXiv e-prints, art. arXiv:1601.02423, Jan. 2016.