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↑  Zaritsky, Dennis; Harris, Jason; Thompson, Ian B.; Grebel, Eva K. (October 2004). “The Magellanic Clouds Photometric Survey: The Large Magellanic Cloud Stellar Catalog and Extinction Map”. 《The Astronomical Journal》 128 (4): 1606–1614. arXiv:astro-ph/0407006. Bibcode:2004AJ....128.1606Z. doi:10.1086/423910. ISSN 0004-6256. S2CID 119532934.
↑  Clark, J. S.; Crowther, P. A.; Larionov, V. M.; Steele, I. A.; Ritchie, B. W.; Arkharov, A. A. (2009). “Bolometric luminosity variations in the luminous blue variable AFGL2298”. 《Astronomy and Astrophysics》 507 (3): 1555–1565. arXiv:0909.4160. Bibcode:2009A&A...507.1555C. doi:10.1051/0004-6361/200912358. S2CID 119187994.
↑  Abdalla, H.; Abramowski, A.; Aharonian, F.; Ait Benkhali, F.; Akhperjanian, A. G.; Angüner, E. O.; Arrieta, M.; Aubert, P.; Backes, M.; Balzer, A.; Barnard, M.; Becherini, Y.; Becker Tjus, J.; Berge, D.; Bernhard, S.; Bernlöhr, K.; Birsin, E.; Blackwell, R.; Böttcher, M.; Boisson, C.; Bolmont, J.; Bordas, P.; Bregeon, J.; Brun, F.; Brun, P.; Bryan, M.; Bulik, T.; Capasso, M.; Carr, J.;  외. (2018). “Extended VHE γ-ray emission towards SGR1806−20, LBV 1806−20, and stellar cluster Cl* 1806−20”. 《Astronomy & Astrophysics》 612: A11. arXiv:1606.05404. Bibcode:2018A&A...612A..11H. doi:10.1051/0004-6361/201628695. S2CID 118345803.
↑  Davies, Ben; de la Fuente, Diego; Najarro, Francisco; Hinton, Jim A.; Trombley, Christine; Figer, Donald F.; Puga, Elena (2012년 1월 21일). “A newly discovered young massive star cluster at the far end of the Galactic Bar: A young cluster at the far end of the Bar”. 《Monthly Notices of the Royal Astronomical Society》 419 (3): 1860–1870. arXiv:1111.2630. Bibcode:2012MNRAS.419.1860D. doi:10.1111/j.1365-2966.2011.19840.x. ISSN 0035-8711. S2CID 59405479.
↑  Niemela, Virpi S.; Shara, Michael M.; Wallace, Debra J.; Zurek, David R.; Moffat, Anthony F. J. (1998). “Hubble Space Telescope Detection of Optical Companions of WR 86, WR 146, and WR 147: Wind Collision Model Confirmed”. 《The Astronomical Journal》 115 (5): 2047–2052. Bibcode:1998AJ....115.2047N. doi:10.1086/300320. S2CID 3606924.
1 2 3  Borissova, J.; Georgiev, L.; Hanson, M. M.; Clarke, J. R. A.; Kurtev, R.; Ivanov, V. D.; Penaloza, F.; Hillier, D. J.; Zsargó, J. (October 2012). “Obscured clusters: IV. The most massive stars in [DBS2003] 179”. 《Astronomy & Astrophysics》 546: A110. arXiv:1209.6370. Bibcode:2012A&A...546A.110B. doi:10.1051/0004-6361/201118348. ISSN 0004-6361. S2CID 119303823.
1 2 3  Borissova, J.; Ivanov, V. D.; Hanson, M. M.; Georgiev, L.; Minniti, D.; Kurtev, R.; Geisler, D. (September 2008). “The young Galactic star cluster [DBS2003] 179”. 《Astronomy & Astrophysics》 488 (1): 151–159. arXiv:0806.4584. Bibcode:2008A&A...488..151B. doi:10.1051/0004-6361:20079255. ISSN 0004-6361. S2CID 14942349.
1 2 3 4 5 6  Bonanos, A. Z.; Lennon, D. J.; Köhlinger, F.; van Loon, J. Th.; Massa, D. L.; Sewilo, M.; Evans, C. J.; Panagia, N.; Babler, B. L.; Block, M.; Bracker, S. (2010년 8월 1일). “Spitzersage-SMC Infrared Photometry of Massive Stars in the Small Magellanic Cloud”. 《The Astronomical Journal》 140 (2): 416–429. arXiv:1004.0949. Bibcode:2010AJ....140..416B. doi:10.1088/0004-6256/140/2/416. hdl:1887/61635. ISSN 0004-6256. S2CID 119290443.
↑  Van Genderen, A. M. (2001). “S Doradus variables in the Galaxy and the Magellanic Clouds”. 《Astronomy and Astrophysics》 366 (2): 508–531. Bibcode:2001A&A...366..508V. doi:10.1051/0004-6361:20000022. Vizie database entry
1 2 3  Bik, A.; Henning, Th.; Wu, S.-W.; Zhang, M.; Brandner, W.; Pasquali, A.; Stolte, A. (April 2019). “Near-infrared spectroscopy of the massive stellar population of W51: evidence for multi-seeded star formation”. 《Astronomy & Astrophysics》 624: A63. arXiv:1902.05460. Bibcode:2019A&A...624A..63B. doi:10.1051/0004-6361/201935061. ISSN 0004-6361. S2CID 118711844.
↑  Egan, Michael P.;  외. (2002). “An Infrared Ring Nebula around MSX5C G358.5391+00.1305: The True Nature of Suspected Planetary Nebula Wray 17-96 Determined via Direct Imaging and Spectroscopy”. 《The Astrophysical Journal》 572 (1): 288–299. Bibcode:2002ApJ...572..288E. doi:10.1086/340222.
↑  Tramper, F.; Sana, H.; Fitzsimons, N. E.; De Koter, A.; Kaper, L.; Mahy, L.; Moffat, A. (2016). “The mass of the very massive binary WR21a”. 《Monthly Notices of the Royal Astronomical Society》 455 (2): 1275–1281. arXiv:1510.03609. Bibcode:2016MNRAS.455.1275T. doi:10.1093/mnras/stv2373. S2CID 44364798.
↑  Oskinova, L. M.; Huenemoerder, D. P.; Hamann, W. -R.; Shenar, T.; Sander, A. A. C.; Ignace, R.; Todt, H.; Hainich, R. (2017). “On the Binary Nature of Massive Blue Hypergiants: High-resolution X-Ray Spectroscopy Suggests That Cyg OB2 12 is a Colliding Wind Binary”. 《The Astrophysical Journal》 845 (1): 39. arXiv:1707.04473. Bibcode:2017ApJ...845...39O. doi:10.3847/1538-4357/aa7e79. S2CID 119537489.
1 2  Laur, Jaan; Kolka, Indrek; Eenmäe, Tõnis; Tuvikene, Taavi; Leedjärv, Laurits (2017). “Variability survey of brightest stars in selected OB associations”. 《Astronomy & Astrophysics》 598: A108. arXiv:1611.02452. Bibcode:2017A&A...598A.108L. doi:10.1051/0004-6361/201629395. ISSN 0004-6361. S2CID 119076598.
1 2 3 4  Moffat, A. F. J. (October 1974). “On the distance and reddening of the massive H II region NGC 3603”. 《Astronomy and Astrophysics》 35: 315. Bibcode:1974A&A....35..315M. ISSN 0004-6361. S2CID 115549707.
↑  Williams, Peredur (2011). “Results from the 2009 campaign on WR 140”. 《Société Royale des Sciences de Liège》 80: 595–609. Bibcode:2011BSRSL..80..595W.
1 2 3  Walborn, N. R.; Morrell, N. I.; Howarth, I. D.; Crowther, P. A.; Lennon, D. J.; Massey, P.; Arias, J. I. (2004). “A CNO Dichotomy among O2 Giant Spectra in the Magellanic Clouds”. 《The Astrophysical Journal》 608 (2): 1028–1038. arXiv:astro-ph/0403557. Bibcode:2004ApJ...608.1028W. doi:10.1086/420761. S2CID 16656083.
1 2  Reed, B. Cameron (2003). “Catalog of Galactic OB Stars”. 《The Astronomical Journal》 125 (5): 2531–2533. Bibcode:2003AJ....125.2531R. doi:10.1086/374771. ISSN 0004-6256. S2CID 121285799.
1 2 3  Humphreys, Roberta M.; Davidson, Kris; Hahn, David; Martin, John C.; Weis, Kerstin (2017년 7월 6일). “Luminous and Variable Stars in M31 and M33 V. The Upper HR Diagram”. 《The Astrophysical Journal》 844 (1): 40. arXiv:1707.01916. Bibcode:2017ApJ...844...40H. doi:10.3847/1538-4357/aa7cef. S2CID 119357524.
↑  Evans, C. J.; Lennon, D. J.; Smartt, S. J.; Trundle, C. (September 2006). “The VLT-FLAMES survey of massive stars: observations centered on the Magellanic Cloud clusters NGC 330, NGC 346, NGC 2004, and the N11 region”. 《Astronomy & Astrophysics》 456 (2): 623–638. arXiv:astro-ph/0606405. Bibcode:2006A&A...456..623E. doi:10.1051/0004-6361:20064988. ISSN 0004-6361. S2CID 13160849.
↑  Smith, Nathan (2006). “A census of the Carina Nebula - I. Cumulative energy input from massive stars”. 《Monthly Notices of the Royal Astronomical Society》 367 (2): 763–772. arXiv:astro-ph/0601060. Bibcode:2006MNRAS.367..763S. doi:10.1111/j.1365-2966.2006.10007.x. S2CID 14060690.
↑  Crowther, Paul A.; Caballero-Nieves, S. M.; Bostroem, K. A.; Maíz Apellániz, J.; Schneider, F. R. N.; Walborn, N. R.; Angus, C. R.; Brott, I.; Bonanos, A.; De Koter, A.; De Mink, S. E.; Evans, C. J.; Gräfener, G.; Herrero, A.; Howarth, I. D.; Langer, N.; Lennon, D. J.; Puls, J.; Sana, H.; Vink, J. S. (2016). “The R136 star cluster dissected with Hubble Space Telescope/STIS. I. Far-ultraviolet spectroscopic census and the origin of He II λ1640 in young star clusters”. 《Monthly Notices of the Royal Astronomical Society》 458 (1): 624–659. arXiv:1603.04994. Bibcode:2016MNRAS.458..624C. doi:10.1093/mnras/stw273.
↑  Massey, Philip (July 2002). “A UBVR CCD Survey of the Magellanic Clouds”. 《The Astrophysical Journal Supplement Series》 141 (1): 81–122. arXiv:astro-ph/0110531. Bibcode:2002ApJS..141...81M. doi:10.1086/338286. ISSN 0067-0049. S2CID 119447348.
↑  Massey, Philip; Olsen, K. A. G.; Hodge, Paul W.; Jacoby, George H.; McNeill, Reagin T.; Smith, R. C.; Strong, Shay B. (2007). “A Survey of Local Group Galaxies Currently Forming Stars. II. UBVRI Photometry of Stars in Seven Dwarfs and a Comparison of the Entire Sample”. 《The Astronomical Journal》 133 (5): 2393–2417. arXiv:astro-ph/0702236. Bibcode:2007AJ....133.2393M. doi:10.1086/513319. ISSN 0004-6256. S2CID 119456878.
↑  Bestenlehner, Joachim M.; Crowther, Paul A.; Broos, Patrick S.; Pollock, Andrew M T.; Townsley, Leisa K. (2022). “Melnick 33Na: A very massive colliding-wind binary system in 30 Doradus”. 《Monthly Notices of the Royal Astronomical Society》 510 (4): 6133–6149. arXiv:2112.00022. Bibcode:2022MNRAS.510.6133B. doi:10.1093/mnras/stab3521.
↑  Castro, N.; Crowther, P. A.; Evans, C. J.; Mackey, J.; Castro-Rodriguez, N.; Vink, J. S.; Melnick, J.; Selman, F. (2018). “Mapping the core of the Tarantula Nebula with VLT-MUSE. I. Spectral and nebular content around R136”. 《Astronomy & Astrophysics》 614: 12. arXiv:1802.01597. Bibcode:2018A&A...614A.147C. doi:10.1051/0004-6361/201732084. S2CID 119341920. A147.
↑  Lamers, H. J. G. L. M. (February 6–10, 1995). 〈Observations and Interpretation of Luminous Blue Variables〉. 《Proceedings of IAU Colloquium 155, Astrophysical applications of stellar pulsation》. 《Astrophysical Applications of Stellar Pulsation. Astronomical Society of the Pacific Conference Series》 83 (Cape Town, South Africa: Astronomical Society of the Pacific). 176–191쪽. Bibcode:1995ASPC...83..176L.
↑  Kastner, J. H.; Buchanan, C. L.; Sargent, B.; Forrest, W. J. (2006). “SpitzerSpectroscopy of Dusty Disks around B\e] Hypergiants in the Large Magellanic Cloud”. 《The Astrophysical Journal》 638 (1): L29–L32. Bibcode:2006ApJ...638L..29K. doi:10.1086/500804.
↑  Humphreys, Roberta M.; Davidson, Kris; Hahn, David; Martin, John C.; Weis, Kerstin (2017년 7월 1일). “Luminous and Variable Stars in M31 and M33. V. The Upper HR Diagram”. 《The Astrophysical Journal》 844 (1): 40. arXiv:1707.01916. Bibcode:2017ApJ...844...40H. doi:10.3847/1538-4357/aa7cef. ISSN 0004-637X. S2CID 119357524.
↑  Aerts, C.; Lefever, K.; Baglin, A.; Degroote, P.; Oreiro, R.; Vučković, M.; Smolders, K.; Acke, B.; Verhoelst, T.; Desmet, M.; Godart, M.; Noels, A.; Dupret, M.-A.; Auvergne, M.; Baudin, F.; Catala, C.; Michel, E.; Samadi, R. (April 2010). “Periodic mass-loss episodes due to an oscillation mode with variable amplitude in the hot supergiant HD 50064”. 《Astronomy and Astrophysics》 513: L11. arXiv:1003.5551. Bibcode:2010A&A...513L..11A. doi:10.1051/0004-6361/201014124. S2CID 41541073.
↑  Taylor, W. D.; Evans, C. J.; Sana, H.; Walborn, N. R.; De Mink, S. E.; Stroud, V. E.; Alvarez-Candal, A.; Barbá, R. H.; Bestenlehner, J. M.; Bonanos, A. Z.; Brott, I.; Crowther, P. A.; De Koter, A.; Friedrich, K.; Gräfener, G.; Hénault-Brunet, V.; Herrero, A.; Kaper, L.; Langer, N.; Lennon, D. J.; Maíz Apellániz, J.; Markova, N.; Morrell, N.; Monaco, L.; Vink, J. S. (2011). “The VLT-FLAMES Tarantula Survey II: R139 revealed as a massive binary system”. 《Astronomy & Astrophysics》 530: L10. arXiv:1103.5387. Bibcode:2011A&A...530L..10T. doi:10.1051/0004-6361/201116785. S2CID 119214376.
↑  Ulaczyk, K.; Szymański, M. K.; Udalski, A.; Kubiak, M.; Pietrzyński, G.; Soszyński, I.; Wyrzykowski, Ł.; Poleski, R.; Gieren, W.; Walker, A. R.; Garcia-Varela, A. (2013년 6월 1일). “Variable Stars from the OGLE-III Shallow Survey in the Large Magellanic Cloud”. 《Acta Astronomica》 63 (2): 159–179. arXiv:1306.4802. Bibcode:2013AcA....63..159U. ISSN 0001-5237. S2CID 119228254.
1 2  Hainich, R.; Pasemann, D.; Todt, H.; Shenar, T.; Sander, A.; Hamann, W. -R (2015). “Wolf-Rayet stars in the Small Magellanic Cloud. I. Analysis of the single WN stars”. 《Astronomy & Astrophysics》 581 (21): 30. arXiv:1507.04000. Bibcode:2015A&A...581A..21H. doi:10.1051/0004-6361/201526241. S2CID 56230998.
↑  Rivero González, J. G.; Puls, J.; Najarro, F.; Brott, I. (2012). “Nitrogen line spectroscopy of O-stars. II. Surface nitrogen abundances for O-stars in the Large Magellanic Cloud”. 《Astronomy & Astrophysics》 537: A79. arXiv:1110.5148. Bibcode:2012A&A...537A..79R. doi:10.1051/0004-6361/201117790. ISSN 0004-6361. S2CID 119110554.
↑  Thompson, Todd A.; Prieto, José L.; Stanek, K. Z.; Kistler, Matthew D.; Beacom, John F.; Kochanek, Christopher S. (2009년 11월 10일). “A New Class of Luminous Transients and a First Census of Their Massive Stellar Progenitors”. 《The Astrophysical Journal》 705 (2): 1364–1384. arXiv:0809.0510. Bibcode:2009ApJ...705.1364T. doi:10.1088/0004-637X/705/2/1364. hdl:1811/48176. ISSN 0004-637X. S2CID 17581579.
↑  Sander, A. A. C.; Hamann, W.-R.; Todt, H.; Hainich, R.; Shenar, T.; Ramachandran, V.; Oskinova, L. M. (2019). “The Galactic WC and WO stars”. 《Astronomy & Astrophysics》 621: A92. arXiv:1807.04293. Bibcode:2019A&A...621A..92S. doi:10.1051/0004-6361/201833712. S2CID 67754788.
1 2  Rauw;  외. (2005년 3월 4일). “The spectrum of the very massive binary system WR 20a (WN6ha + WN6ha): Fundamental parameters and wind interactions”. 《Astronomy & Astrophysics》 432 (3): 985–998. Bibcode:2005A&A...432..985R. doi:10.1051/0004-6361:20042136.
1 2  Peeples, Molly S.; Bonanos, A. Z.; DePoy, D. L.; Stanek, K. Z.; Pepper, J.; Pogge, Richard W.; Pinsonneault, M. H.; Sellgren, K. (2007년 1월 1일). “The Nature of the Variable Galactic Center Source GCIRS 16SW Revisited: A Massive Eclipsing Binary”. 《The Astrophysical Journal》 654 (1): L61–L64. arXiv:astro-ph/0610212. Bibcode:2007ApJ...654L..61P. doi:10.1086/510720. ISSN 0004-637X. S2CID 14242573.
↑  Morrell, N. I.; Barbá, R. H.; Niemela, V. S.; Corti, M. A.; Albacete Colombo, J. F.; Rauw, G.; Corcoran, M.; Morel, T.; Bertrand, J.-F.; Moffat, A. F. J.; St-Louis, N. (2001). “Optical spectroscopy of X-Mega targets - II. The massive double-lined O-type binary HD 93205”. 《Monthly Notices of the Royal Astronomical Society》 326 (1): 85–94. arXiv:astro-ph/0105014. Bibcode:2001MNRAS.326...85M. doi:10.1046/j.1365-8711.2001.04500.x. S2CID 16221731.
1 2  Neugent, Kathryn F.; Massey, Philip (2011년 6월 1일). “The Wolf-Rayet Content of M33”. 《The Astrophysical Journal》 733 (2): 123. arXiv:1103.5549. Bibcode:2011ApJ...733..123N. doi:10.1088/0004-637X/733/2/123. ISSN 0004-637X. S2CID 118507918.
↑  Walborn, N. R.; Sana, H.; Simón-Díaz, S.; Maíz Apellániz, J.; Taylor, W. D.; Evans, C. J.; Markova, N.; Lennon, D. J.; de Koter, A. (2014). “The VLT-FLAMES Tarantula Survey. XIV. The O-type stellar content of 30 Doradus”. 《Astronomy & Astrophysics》 564 (40): 35. arXiv:1402.6969. Bibcode:2014A&A...564A..40W. doi:10.1051/0004-6361/201323082. S2CID 119302111.
↑  Rauw, G.; Vreux, J.-M.; Stevens, I. R.; Gosset, E.; Sana, H.; Jamar, C.; Mason, K. O. (2002). “Phase-resolved X-ray and optical spectroscopy of the massive binary HD 93403”. 《Astronomy and Astrophysics》 388 (2): 552. Bibcode:2002A&A...388..552R. doi:10.1051/0004-6361:20020523.
↑  Crowther, P. A.; Hadfield, L. J.; Clark, J. S.; Negueruela, I.; Vacca, W. D. (2006년 11월 1일). “A census of the Wolf-Rayet content in Westerlund 1 from near-infrared imaging and spectroscopy”. 《Monthly Notices of the Royal Astronomical Society》 372 (3): 1407–1424. arXiv:astro-ph/0608356. Bibcode:2006MNRAS.372.1407C. doi:10.1111/j.1365-2966.2006.10952.x. ISSN 0035-8711. S2CID 10505573.
↑  Clark, J. S.; Muno, M. P.; Negueruela, I.; Dougherty, S. M.; Crowther, P. A.; Goodwin, S. P.; de Grijs, R. (2008). “Unveiling the X-ray point source population of the Young Massive Cluster Westerlund 1”. 《Astronomy & Astrophysics》 477 (1): 147–163. Bibcode:2008A&A...477..147C. doi:10.1051/0004-6361:20077186. ISSN 0004-6361.
1 2 3 4  Repolust, T.; Puls, J.; Herrero, A. (2004). “Stellar and wind parameters of Galactic O-stars. The influence of line-blocking/blanketing”. 《Astronomy and Astrophysics》 415: 349. Bibcode:2004A&A...415..349R. doi:10.1051/0004-6361:20034594.
↑  Neugent, Kathryn F.; Massey, Philip; Morrell, Nidia (2012년 12월 1일). “The Discovery of a Rare Wo-Type Wolf–Rayet Star in the Large Magellanic Cloud”. 《The Astronomical Journal》 144 (6): 162. arXiv:1210.0062. Bibcode:2012AJ....144..162N. doi:10.1088/0004-6256/144/6/162. ISSN 0004-6256. S2CID 118628394.
↑  Clark, J. S.; Najarro, F.; Negueruela, I.; Ritchie, B. W.; Urbaneja, M. A.; Howarth, I. D. (2012). “On the nature of the galactic early-B hypergiants”. 《Astronomy & Astrophysics》 541: A145. arXiv:1202.3991. Bibcode:2012A&A...541A.145C. doi:10.1051/0004-6361/201117472. ISSN 0004-6361. S2CID 11978733.
↑  Kozok, J. R. (September 1985), “Photometric observations of emission B-stars in the southern Milky Way”, 《Astronomy and Astrophysics Supplement Series》 61: 387–405, Bibcode:1985A&AS...61..387K
1 2  Bouret, J. -C.; Hillier, D. J.; Lanz, T.; Fullerton, A. W. (2012). “Properties of Galactic early-type O-supergiants: A combined FUV-UV and optical analysis”. 《Astronomy & Astrophysics》 544: A67. arXiv:1205.3075. Bibcode:2012A&A...544A..67B. doi:10.1051/0004-6361/201118594. S2CID 119280104.
↑  Rivet, J-P; Siciak, A.; de Almeida, E. S. G.; Vakili, F.; Domiciano de Souza, A.; Fouché, M.; Lai, O.; Vernet, D.; Kaiser, R.; Guerin, W. (2020). “Intensity interferometry of P Cygni in the H α emission line: Towards distance calibration of LBV supergiant stars”. 《Monthly Notices of the Royal Astronomical Society》 494 (1): 218–227. arXiv:1910.08366. Bibcode:2020MNRAS.494..218R. doi:10.1093/mnras/staa588. S2CID 204788654.
↑  Skinner, Stephen L.; Zhekov, Svetozar A.; Güdel, Manuel; Schmutz, Werner; Sokal, Kimberly R. (2012년 5월 1일). “New X-Ray Detections of WNL Stars”. 《The Astronomical Journal》 143 (5): 116. arXiv:1203.5098. Bibcode:2012AJ....143..116S. doi:10.1088/0004-6256/143/5/116. ISSN 0004-6256. S2CID 119281411.
1 2 3  Searle, S. C.; Prinja, R. K.; Massa, D.; Ryans, R. (2008). “Quantitative studies of the optical and UV spectra of Galactic early B supergiants. I. Fundamental parameters”. 《Astronomy and Astrophysics》 481 (3): 777–97. arXiv:0801.4289. Bibcode:2008A&A...481..777S. doi:10.1051/0004-6361:20077125. S2CID 1552752.
↑  Mehner, Andrea; Davidson, Kris; Ferland, Gary J.; Humphreys, Roberta M. (2010). “High-excitation Emission Lines near Eta Carinae, and Its Likely Companion Star”. 《The Astrophysical Journal》 710 (1): 729–742. arXiv:0912.1067. Bibcode:2010ApJ...710..729M. doi:10.1088/0004-637X/710/1/729. S2CID 5032987.
↑  Lefever, K.; Puls, J.; Aerts, C. (2007). “Statistical properties of a sample of periodically variable B-type supergiants: Evidence for opacity-driven gravity-mode oscillations”. 《Astronomy & Astrophysics》 463 (3): 1093–1109. arXiv:astro-ph/0611484. Bibcode:2007A&A...463.1093L. doi:10.1051/0004-6361:20066038. ISSN 0004-6361. S2CID 8783008.
1 2 3 4 5 6  Hohle, M. M.; Neuhäuser, R.; Schutz, B. F. (April 2010), “Masses and luminosities of O- and B-type stars and red supergiants”, 《Astronomische Nachrichten》 331 (4): 349, arXiv:1003.2335, Bibcode:2010AN....331..349H, doi:10.1002/asna.200911355, S2CID 111387483
↑  Sugawara, Y.; Tsuboi, Y.; Maeda, Y. (October 2008). “Redshifted emission lines and radiative recombination continuum from the Wolf-Rayet binary θ Muscae: evidence for a triplet system?”. 《Astronomy & Astrophysics》 490 (1): 259–264. arXiv:0810.1208. Bibcode:2008A&A...490..259S. doi:10.1051/0004-6361:20079302. ISSN 0004-6361. S2CID 118447784.
1 2  North, J. R.; Tuthill, P. G.; Tango, W. J.; Davis, J. (2007년 5월 1일). “γ2 Velorum: orbital solution and fundamental parameter determination with SUSI”. 《Monthly Notices of the Royal Astronomical Society》 377 (1): 415–424. arXiv:astro-ph/0702375. Bibcode:2007MNRAS.377..415N. doi:10.1111/j.1365-2966.2007.11608.x. ISSN 0035-8711. S2CID 16425744.
↑  Hummel, C. A.; Rivinius, Th.; Nieva, M.-F.; Stahl, O.; van Belle, G.; Zavala, R. T. (2013). “Dynamical mass of the O-type supergiant in ζ Orionis A”. 《Astronomy & Astrophysics》 554: A52. arXiv:1306.0330. Bibcode:2013A&A...554A..52H. doi:10.1051/0004-6361/201321434. ISSN 0004-6361. S2CID 53645495.
↑  Nugis, T.; Lamers, H. J. G. L. M. (2000). “Mass-loss rates of Wolf-Rayet stars as a function of stellar parameters”. 《Astronomy and Astrophysics》 360: 227. Bibcode:2000A&A...360..227N.