A comprehensive search for hot subdwarf stars using Gaia and TESS
Astronomy & AstrophysicsHot subdwarf B (sdB) stars are evolved, subluminous, helium-burning stars that most likely form when red giant stars loose their hydrogen envelope via interactions with close companions. They play an important role in our understanding of binary evolution, stellar atmospheres, and interiors.
Murat Uzundag +7 more
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Hot Subdwarf Stars Identified in Gaia DR2 with Spectra of LAMOST DR6 and DR7. I. Single-lined Spectra [PDF]
, 2020 Zhenxin Lei +3 more
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The evolution of a hot subdwarf: observations of the pulsating subdwarf B star Feige~48
, 2003 Since pulsating subdwarf B (sdBV or EC14026) stars were first discovered (Kilkenny et al, 1997), observational efforts have tried to realize their potential for constraining the interior physics of extreme horizontal branch (EHB) stars. Difficulties encountered along the way include uncertain mode identifications and a lack of stable pulsation mode ...
Reed, M. D. +2 more
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Hot subdwarf stars and their connection to thermonuclear supernovae [PDF]
, 2016 Stephan Geier +12 more
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Follow-up observations of X-ray emitting hot subdwarf stars: the He-rich sdO BD +37° 1977 [PDF]
, 2015 N. La Palombara +4 more
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The composition of Kapteyn's star and the M subdwarfs.
The Astrophysical Journal, 1976 The metal abundance of the nearby M subdwarf Kapteyn's star is obtained from a 10 A mm/sup -1/ spectrum in the near-infrared. The weighted mean value of (M/H) is -0.55 +- 0.15 (p.e.), confirming an earlier estimate from the strength of the TiO bands. The O/C ratio in Kapteyn's star is within a factor of 2 of the solar value.
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Are Analogues of Hot Subdwarf Stars Responsible for the UVX Phenomenon in Galaxy Nuclei? [PDF]
, 1994 Ben Dorman +2 more
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On the Capability of Oxidovanadium(IV) Derivatives to Act as All-Around Catalytic Promoters Since the Prebiotic World. [PDF]
Molecules, 2020 Campitelli P, Crucianelli M.
europepmc +1 more source
Optical spectroscopy of high proper motion stars: new M dwarfs within 10 pc and the closest pair of subdwarfs [PDF]
, 2006 C. Reylé +4 more
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