Results 21 to 30 of about 51,217 (241)

Astrometric Binary Classification via Artificial Neural Networks [PDF]

open access: yesThe Astrophysical Journal
With nearly two billion stars observed and their corresponding astrometric parameters evaluated in the recent Gaia mission, the number of astrometric binary candidates has risen significantly.
Joe Smith
doaj   +2 more sources

Seismic inference of 57 stars using full-length Kepler data sets [PDF]

open access: yesEPJ Web of Conferences, 2017
We present stellar properties of 57 stars from a seismic inference using full-length data sets from Kepler (mass, age, radius, distances). These stars comprise active stars, planet-hosts, solar-analogs, and binary systems.
Creevey Orlagh   +8 more
doaj   +3 more sources

Mining of the Milky Way Star Archive Gaia-DR2. Searching for Binary Stars in Planetary Nebulae

open access: yesProceedings, 2020
The aim of this work is to search for binary stars associated to planetary nebulae (ionized stellar envelopes in expansion), by mining the astronomical archive of Gaia DR2, that is composed by around 1.7 billion stellar sources.
Iker González-Santamaría   +4 more
doaj   +2 more sources

Planetary systems in close binary stars: the case of HD 196885 [PDF]

open access: yesAstronomy & Astrophysics, 2011
Context. More than fifty candidate planets are presently known to orbit one component of a binary or a multiple star system. Planets can therefore form and survive in such an environment, although recent observing surveys indicate that short-separation binaries do not favour the presence of a planetary system around one of the components.
Chauvin G   +3 more
openaire   +3 more sources

A Binary Origin for the First Isolated Stellar-mass Black Hole Detected with Astrometric Microlensing [PDF]

open access: yesThe Astrophysical Journal Letters, 2023
The Milky Way is believed to host hundreds of millions of quiescent stellar-mass black holes (BHs). In the last decade, some of these objects have been potentially uncovered via gravitational microlensing events.
Alejandro Vigna-Gómez   +1 more
doaj   +2 more sources

Visual Orbits of Wolf–Rayet Stars. I. The Orbit of the Dust-producing Wolf–Rayet Binary WR 137 Measured with the CHARA Array

open access: yesThe Astrophysical Journal
Classical Wolf–Rayet (W-R) stars are the descendants of massive OB stars that have lost their hydrogen envelopes and are burning helium in their cores prior to exploding as Type Ib/c supernovae.
Noel D. Richardson   +21 more
doaj   +2 more sources

Orbital Inclination of Astrometric Binaries and the Dearth of Face-on Orbits in Gaia DR3 Solutions

open access: yesThe Astrophysical Journal Letters
The orbital solutions for astrometric (unresolved) binary stars provided in the Gaia mission DR3 reveal an obvious deficit of face-on orbits with line-of-sight inclinations close to 0 or π .
Valeri V. Makarov
doaj   +2 more sources

Disk Evolution Study Through Imaging of Nearby Young Stars (DESTINYS): Diverse outcomes of binary-disk interactions [PDF]

open access: yesAstronomy & Astrophysics, 2023
Circumstellar disks do not evolve in isolation, as about half of solar-type stars were born in binary or multiple systems. Resolving disks in binary systems provides the opportunity to examine the influence of stellar companions on the outcomes of planet
Yapeng Zhang   +17 more
semanticscholar   +1 more source

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