Results 21 to 30 of about 618,458 (224)
SDSS J0926+3624 : the shortest period eclipsing binary star [PDF]
With orbital periods of the order of tens of minutes or less, the AM Canum Venaticorum stars are ultracompact, hydrogen-deficient binaries with the shortest periods of any binary subclass, and are expected to be among the strongest gravitational wave ...
Roelofs, Gijs H. A. +44 more
core +2 more sources
In this study, we identify 11 Kepler systems (KIC 5255552, 5653126, 5731312, 7670617, 7821010, 8023317, 10268809, 10296163, 11519226, 11558882, and 12356914) with a flip-flop effect in the eclipse timing variations O - C diagrams of the systems, report ...
O'Toole, S.O. +3 more
core +1 more source
A window into δ Sct stellar interiors: understanding the eclipsing binary system TT Hor [PDF]
<p>MESA inlists associated with <a href="https://ui.adsabs.harvard.edu/#abs/2018MNRAS.480.1372S/abstract">A window into δ Sct stellar interiors: understanding the eclipsing binary system TT Hor</a></p ...
Bento, Joao +10 more
core +1 more source
: A new eclipsing sdB binary [PDF]
We report the discovery of an eclipsing binary -HS 0705 ...
R. Napiwotzki +8 more
core +1 more source
A Search for Exoplanets in Short-Period Binary Star Systems [PDF]
This paper reports the progress of a search for exoplanets with S-type orbits in short-period binary star systems. The selected targets have stellar orbital periods of just a few days. These systems are eclipsing binaries so that exoplanet transits, if
Ronald Kaitchuck +2 more
doaj +1 more source
A transiting companion to the eclipsing binary KIC002856960
We present an early result from an automated search of Kepler eclipsing binary systems for circumbinary companions. An intriguing tertiary signal has been discovered in the short period eclipsing binary KIC002856960. This third body leads to transit-like
Gómez Maqueo Chew, Y. +26 more
core +3 more sources
Eclipsing binary stars with a delta Scuti component [PDF]
Eclipsing binaries with a d Sct component are powerful tools to derive the fundamental parameters and probe the internal structure of stars. In this study, spectral analysis of six primary d Sct components in eclipsing binaries has been performed. Values
Smalley
core +1 more source
Accurate fundamental parameters of eclipsing binary stars [PDF]
The study of detached eclipsing binaries is one of the most powerful ways to investigate the properties of individual stars and stellar systems. We present preliminary masses, radii and effective temperatures for the eclipsing binary WW Aurigae, which is
Maxted, Pierre +11 more
core +1 more source
The Transiting Exoplanet Survey Satellite (TESS) has surveyed nearly the entire sky in full-frame image mode with a time resolution of 200 s to 30 minutes and a temporal baseline of at least 27 days.
Veselin B. Kostov +38 more
doaj +1 more source
Close-In Substellar Companions and the Formation of sdB-Type Close Binary Stars
The sdB-type close binaries are believed to have experienced a common-envelope phase and may evolve into cataclysmic binaries (CVs). About 10% of all known sdB binaries are eclipsing binaries consisting of very hot subdwarf primaries and low-mass ...
L. Y. Zhu +4 more
doaj +1 more source

