Results 11 to 20 of about 221,937 (281)

Fundamental parameters of the Ap-stars GO And, 84 UMa, and κ Psc [PDF]

open access: yesAstronomy & Astrophysics, 2021
Aims. The aim of this work is to determine fundamental parameters of three Ap stars, GO And (HD 4778), κ Psc (HD 220825), and 84 UMa (HD 120198), using spectroscopic techniques. By analysing these stars, we complete the sample of Ap stars for which fundamental parameters have additionally been derived by means of interferometry.
A. M. Romanovskaya   +3 more
semanticscholar   +6 more sources

Fundamental parameters and infrared excesses of Tycho–Gaia stars [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2017
43 pages, 50 figures, accepted ...
McDonald, I, Watson, RA, Zijlstra, AA
semanticscholar   +8 more sources

Atmospheric and Fundamental Parameters of Eight Nearby Multiple Stars

open access: yesThe 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
semanticscholar   +4 more sources

Fundamental parameters and infrared excesses of Hipparcos stars [PDF]

open access: yesRoyal Astronomical Society. Monthly Notices, 2012
We derive the fundamental parameters (temperature and luminosity) of 107 619 Hipparcos stars and place these stars on a true Hertzsprung-Russell diagram. This is achieved by comparing BT-Settl model atmospheres to spectral energy distributions (SEDs) created from Hipparcos, Tycho, SDSS, DENIS, 2MASS, MSX, AKARI, IRAS and WISE data. We also identify and
Mcdonald, I.   +2 more
semanticscholar   +5 more sources

Fundamental parameters of Be stars located in the seismology fields of COROT [PDF]

open access: yesAstronomy & Astrophysics, 2006
25 pages, 9 figures, Accepted for publication in A& ...
Frémat, Yves   +6 more
semanticscholar   +8 more sources

Gaia FGK benchmark stars: Fundamental Teff and logg of the third version [PDF]

open access: yesAstronomy & Astrophysics, 2023
Large spectroscopic surveys devoted to the study of the Milky Way, including Gaia, use automated pipelines to determine the atmospheric parameters of millions of stars. The Gaia FGK benchmark stars are reference stars with and derived through fundamental
C. Soubiran   +10 more
semanticscholar   +2 more sources

THE PAN-PACIFIC PLANET SEARCH. V. FUNDAMENTAL PARAMETERS FOR 164 EVOLVED STARS [PDF]

open access: yes, 2016
We present spectroscopic stellar parameters for the complete target list of 164 evolved stars from the Pan-Pacific Planet Search, a five-year radial velocity campaign using the 3.9 m Anglo-Australian Telescope.
R. Wittenmyer   +5 more
semanticscholar   +3 more sources

Fundamental parameters of massive stars [PDF]

open access: yesEAS Publications Series, 2004
21 pages, 3 figures, to appear in "Massive Stars: Formation, Evolution and Environment", eds. Heydari-Malayeri & Zahn (proceedings of 2002 Aussois summer school)
P. A. Crowther
openaire   +3 more sources

FUNDAMENTAL PARAMETERS OF MAIN-SEQUENCE STARS IN AN INSTANT WITH MACHINE LEARNING [PDF]

open access: yesThe 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
openaire   +6 more sources

Fundamental stellar parameters of benchmark stars from CHARA interferometry [PDF]

open access: yesAstronomy & Astrophysics, 2020
Context.Benchmark stars are crucial as validating standards for current as well as future large stellar surveys of the Milky Way. However, the number of suitable metal-poor benchmark stars is currently limited, owing to the difficulty in determining reliable effective temperatures (Teff) in this regime.Aims.We aim to construct a new set of metal-poor ...
I. Karovicova   +6 more
core   +4 more sources

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