Results 131 to 140 of about 4,387 (203)
Subdwarfs. II - The missing halo-population K subdwarfs
The Astrophysical Journal, 1979 M. S. Bessell, D. T. Wickramasinghe
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, 1963 HD 49798 was found to be a hot subdwarf. It is, at the present time the brightest member of this group and also the only one known spectroscopic binary. The complete paper will appear in the "Publications of the Astronomical Society of the Pacific".
Jaschek, Mercedes, Jaschek, Carlos
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Detection of the Progenitors of Be X-ray Binaries. [PDF]
Proc Int Astron Union, 2018 Gies D, Wang L, Peters G.
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A Brown Dwarf Orbiting around the Planetary-nebula Central Binary KV Vel
The Astrophysical JournalKV Vel is a noneclipsing short-period ( P = 0.3571 days) close binary containing a very hot subdwarf primary (77,000 K) and a cool low-mass secondary star (3400 K) that is located at the center of the planetary nebula DS 1.
S.-B. Qian +11 more
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Photometric variability in four hot subdwarf stars [PDF]
, 2016 D. Kilkenny, C. Koen
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A Kinematically Cold Structure of Candidate Young OB Stars toward the Anticenter. [PDF]
Astrophys J, 2019 Casetti-Dinescu DI, Girard TM.
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Citation-based clustering of publications using CitNetExplorer and VOSviewer. [PDF]
Scientometrics, 2017 van Eck NJ, Waltman L.
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A Search for Subdwarf B Binaries Using Pulsation Timing from TESS
The Astronomical JournalHot subdwarf B (sdB) stars are post-main-sequence stars of high temperature and gravity. Approximately 30% of sdBs exhibit stable pressure and/or gravity-mode pulsations, which can be used via the timing method to test for companion stars and determine ...
Tomomi Otani +5 more
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