Results 121 to 130 of about 6,211 (193)

The O-C diagram of the subdwarf B pulsating star HS2201+2610: detection of a giant planet? [PDF]

open access: green, 2007
R. Silvotti   +11 more
openalex   +1 more source

Some Subdwarf Models

open access: yes, 1962
In this paper we present the results obtained from the numerical integration of the equations for the case of subdwarfs with masses comparable and somewhat larger than that of the Sun.
Varsavsky, Carlos Manuel   +2 more
openaire   +1 more source

Accurate mass and radius determinations of a cool subdwarf in an eclipsing binary. [PDF]

open access: yesNat Astron, 2019
Rebassa-Mansergas A   +6 more
europepmc   +1 more source

The hot subdwarf B + white dwarf binary KPD 1930+2752 - a Supernova Type Ia progenitor candidate [PDF]

open access: green, 2006
S. Geier   +5 more
openalex   +1 more source

Hot Subdwarfs in Binaries as the Source of the Far-UV Excess in Elliptical Galaxies [PDF]

open access: green, 2008
Philipp Podsiadlowski   +3 more
openalex   +1 more source

The EXOTIME project: signals in the O–C diagrams of the rapidly pulsating subdwarfs DW Lyn, V1636 Ori, QQ Vir, and V541 Hya [PDF]

open access: hybrid, 2020
F. Mackebrandt   +19 more
openalex   +1 more source

A Brown Dwarf Orbiting around the Planetary-nebula Central Binary KV Vel

open access: yesThe Astrophysical Journal
KV 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
doaj   +1 more source

Detection of the Progenitors of Be X-ray Binaries. [PDF]

open access: yesProc Int Astron Union, 2018
Gies D, Wang L, Peters G.
europepmc   +1 more source

A Search for Subdwarf B Binaries Using Pulsation Timing from TESS

open access: yesThe Astronomical Journal
Hot 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
doaj   +1 more source

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