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Fundamental Parameters of CP Stars [PDF]
Highlights of Astronomy, 1998 The quest for accurate fundamental parameters (M, R, Teff log g, v sin i) of CP stars has been a lasting problem ever since the nature and origin of these stars has been discussed. The main reason for the difficulty lies in the anomalous colours of these stars, linked with their abundance anomalies which are responsible for complicated blocking and ...
P. North
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Fundamental stellar parameters of benchmark stars from CHARA interferometry -- III. Giant and subgiant stars [PDF]
Astronomy & Astrophysics, 2021 Context.Large spectroscopic surveys of the Milky Way must be calibrated against a sample of benchmark stars to ensure the reliable determination of atmospheric parameters.Aims.Here, we present new fundamental stellar parameters of seven giant and subgiant stars that will serve as benchmark stars for large surveys.
I. Karovicova +5 more
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Fundamental parameters and infrared excesses of Tycho–Gaia stars [PDF]
Monthly Notices of the Royal Astronomical Society, 2017 43 pages, 50 figures, accepted ...
Iain McDonald +2 more
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Fundamental stellar parameters of benchmark stars from CHARA interferometry -- II. Dwarf stars [PDF]
Astronomy & Astrophysics, 2021 Context. Stellar models applied to large stellar surveys of the Milky Way need to be properly tested against a sample of stars with highly reliable fundamental stellar parameters. We have established a programme aiming to deliver such a sample of stars. Aims.
I. Karovicova +5 more
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Accurate fundamental parameters of eclipsing binary stars [PDF]
Proceedings of the International Astronomical Union, 2004 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 composed of two metallic-lined A-type stars.
J. Southworth +3 more
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Fundamental parameters of B type stars [PDF]
Proceedings of the International Astronomical Union, 2014 AbstractFundamental parameters of 26 well-studied sharp-lined single early B-type stars in OB associations and in the field within a distance of ≤400 pc from the Sun are compared to high-precision data from detached eclipsing binaries (DEBs). Fundamental parameters are derived from accurate and precise atmospheric parameters determined earlier by us ...
María-Fernanda Nieva
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Atmospheric and Fundamental Parameters of Eight Nearby Multiple Stars
The Astronomical Journal, 2022 Abstract We present the complete set of atmospheric and fundamental parameters, in addition to the masses, for the individual components of eight stellar systems. The list of the systems, whose orbital solutions were published recently, includes seven binaries (HIP 14524, HIP 16025, HIP 46199, HIP 47791, HIP 60444, HIP 61100, HIP 73085 ...
Abdallah M. Hussein +6 more
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FUNDAMENTAL PARAMETERS OF MAIN-SEQUENCE STARS IN AN INSTANT WITH MACHINE LEARNING [PDF]
The Astrophysical Journal, 2016 ABSTRACT Owing to the remarkable photometric precision of space observatories like Kepler, stellar and planetary systems beyond our own are now being characterized en masse for the first time. These characterizations are pivotal for endeavors such as searching for Earth-like planets and solar twins, understanding the mechanisms that ...
Earl P. Bellinger +5 more
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Using limb darkening to measure fundamental parameters of stars [PDF]
Astronomy & Astrophysics, 2012 Context. Limb darkening is an important tool for understanding stellar atmospheres, but most observations measuring limb darkening assume various parameterizations that yield no significant information about the structure of stellar atmospheres. Aims. We use a specific limb-darkening relation to study how the best-fit coefficients relate to fundamental
H. R. Neilson, J. B. Lester
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Asteroseismic Determination of Fundamental Parameters for Exoplanet Host Stars with Deep Learning
Astronomy and Computing, 2022 Asteroseismology — techniquesNeural network — starsOscillations — starsFundamental ...
Zihan Guo, Chen Jiang
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