WOH G64 (German Wikipedia)

Analysis of information sources in references of the Wikipedia article "WOH G64" in German language version.

refsWebsite
Global rank German rank
2nd place
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6th place
1,342nd place
799th place

doi.org

  • Emily M. Levesque, Philip Massey, Bertrand Plez, Knut A. G. Olsen: THE PHYSICAL PROPERTIES OF THE RED SUPERGIANT WOH G64: THE LARGEST STAR KNOWN? In: The Astronomical Journal. Band 137, Nr. 6, 1. Juni 2009, ISSN 0004-6256, S. 4744–4752, doi:10.1088/0004-6256/137/6/4744.
  • S. de Wit, A.Z. Bonanos, F. Tramper, M. Yang, G. Maravelias, K. Boutsia, N. Britavskiy, E. Zapartas: Properties of luminous red supergiant stars in the Magellanic Clouds. In: Astronomy & Astrophysics. Band 669, Januar 2023, ISSN 0004-6361, S. A86, doi:10.1051/0004-6361/202243394.
  • Emily M Levesque: Physical Properties of Red Supergiants. In: Astrophysics of Red Supergiants. IOP Publishing, 2017, ISBN 978-0-7503-1329-2, S. 3–1–3–13, doi:10.1088/978-0-7503-1329-2ch3.
  • Emma R. Beasor, Nathan Smith: The Extreme Scarcity of Dust-enshrouded Red Supergiants: Consequences for Producing Stripped Stars via Winds. In: The Astrophysical Journal. Band 933, Nr. 1, 1. Juli 2022, ISSN 0004-637X, S. 41, doi:10.3847/1538-4357/ac6dcf.

u-strasbg.fr

vizier.u-strasbg.fr

zdb-katalog.de

  • Emily M. Levesque, Philip Massey, Bertrand Plez, Knut A. G. Olsen: THE PHYSICAL PROPERTIES OF THE RED SUPERGIANT WOH G64: THE LARGEST STAR KNOWN? In: The Astronomical Journal. Band 137, Nr. 6, 1. Juni 2009, ISSN 0004-6256, S. 4744–4752, doi:10.1088/0004-6256/137/6/4744.
  • S. de Wit, A.Z. Bonanos, F. Tramper, M. Yang, G. Maravelias, K. Boutsia, N. Britavskiy, E. Zapartas: Properties of luminous red supergiant stars in the Magellanic Clouds. In: Astronomy & Astrophysics. Band 669, Januar 2023, ISSN 0004-6361, S. A86, doi:10.1051/0004-6361/202243394.
  • Emma R. Beasor, Nathan Smith: The Extreme Scarcity of Dust-enshrouded Red Supergiants: Consequences for Producing Stripped Stars via Winds. In: The Astrophysical Journal. Band 933, Nr. 1, 1. Juli 2022, ISSN 0004-637X, S. 41, doi:10.3847/1538-4357/ac6dcf.