Support for a white dwarf in the Be star binary 
Cassiopeiae
A&A, 382 2 (2002) 554-555
Published online: 2002-02-15
Articles citing this article
The Citing articles tool gives a list of articles citing the current article.
The citing articles come from EDP Sciences database, as well as other publishers participating in CrossRef Cited-by Linking Program. You can set up your personal account to receive an email alert each time this article is cited by a new article (see the menu on the right-hand side of the abstract page).
Cited article:
Support for a white dwarf in the Be star binary
This article has been cited by the following article(s):
High energy emission powered by accreting companions of Be/$\gamma $ Cas stars
Rina G. Rast, Yaël Nazé, Jonathan Labadie-Bartz, Carol E. Jones, Christiana Erba, Ken Gayley, Asif ud-Doula, Coralie Neiner and Jeremy J. DrakeAstrophysics and Space Science 370 (10) (2025)
https://doi.org/10.1007/s10509-025-04497-6
The X-ray Emission of γ Cassiopeiae During the 2020–2021 disc eruption
G. Rauw, Y. Nazé, C. Motch, et al.Astronomy & Astrophysics 664 A184 (2022)
https://doi.org/10.1051/0004-6361/202243679
Suzaku and NuSTAR X-ray spectroscopy of γ Cassiopeiae and HD 110432
Masahiro Tsujimoto, Kumiko Morihana, Takayuki Hayashi and Takao KitaguchiPublications of the Astronomical Society of Japan 70 (6) (2018)
https://doi.org/10.1093/pasj/psy111
A propelling neutron star in the enigmatic Be-star γ Cassiopeia
K. Postnov, L. Oskinova and J. M. TorrejónMonthly Notices of the Royal Astronomical Society: Letters 465 (1) L119 (2017)
https://doi.org/10.1093/mnrasl/slw223
The X-ray emission of the γ Cassiopeiae stars
Myron A. Smith, R. Lopes de Oliveira and C. MotchAdvances in Space Research 58 (5) 782 (2016)
https://doi.org/10.1016/j.asr.2015.12.032
HIGH-ENERGY PROPERTIES OF THE ENIGMATIC Be STAR γ CASSIOPEIAE
C. R. Shrader, K. Hamaguchi, S. J. Sturner, et al.The Astrophysical Journal 799 (1) 84 (2015)
https://doi.org/10.1088/0004-637X/799/1/84
On the feasibility of detection of neutron star companions to OB runaways using Gaia astrometry
Cóilín Ó Maoiléidigh, Evert J.A. Meurs and Laura NorciNew Astronomy 10 (7) 591 (2005)
https://doi.org/10.1016/j.newast.2005.03.002
High‐ResolutionChandraSpectroscopy of γ Cassiopeiae (B0.5e)
Myron A. Smith, David H. Cohen, Ming Feng Gu, et al.The Astrophysical Journal 600 (2) 972 (2004)
https://doi.org/10.1086/379873
Rotational mass loss by Be stars
A. V. Tutukov and A. V. FedorovaAstronomy Reports 47 (10) 826 (2003)
https://doi.org/10.1134/1.1618994