Results 1 to 10 of about 188,912 (128)

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

open access: bronzeAstronomy & 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 funda-
A. M. Romanovskaya   +3 more
openalex   +3 more sources

Fundamental parameters and evolutionary status of the magnetic chemically peculiar stars HD 188041 (V1291 Aquilae), HD 111133 (EP Virginis), and HD 204411: spectroscopy versus interferometry [PDF]

open access: bronzeMonthly notices of the Royal Astronomical Society, 2019
The determination of fundamental parameters of stars is one of the main tasks of astrophysics. For magnetic chemically peculiar stars, this problem is complicated by the anomalous chemical composition of their atmospheres, which requires special ...
A. M. Romanovskaya   +6 more
openalex   +3 more sources

Fundamental parameters of massive stars in multiple systems: The cases of HD 17505A and HD 206267A [PDF]

open access: bronzeAstronomy & Astrophysics, 2018
Context. Many massive stars are part of binary or higher multiplicity systems. The present work focusses on two higher multiplicity systems: HD 17505A and HD 206267A. Aims.
F. Raucq   +7 more
openalex   +3 more sources

Angular Diameters and Fundamental Parameters of Forty-four Stars from the Navy Precision Optical Interferometer [PDF]

open access: bronzeAstronomical Journal, 2021
We measured the angular diameters of 44 stars with the Navy Precision Optical Interferometer, obtaining uncertainties on the limb-darkened diameter of 2% or less for all but four stars.
Ellyn K. Baines   +11 more
openalex   +3 more sources

VLTI/AMBER observations of cold giant stars: atmospheric structures and fundamental parameters [PDF]

open access: bronze, 2014
Aims. The main goal of this research is to determine the angular size and the atmospheric structures of cool giant stars (epsilon Oct, beta Peg, NU Pav, psi Peg, and gamma Hya) and to compare them with hydrostatic stellar model atmospheres, to estimate ...
B. Arroyo-Torres   +14 more
openalex   +3 more sources

When a period is not a full stop: Light-curve structure reveals fundamental parameters of Cepheid and RR Lyrae stars [PDF]

open access: bronzeMonthly notices of the Royal Astronomical Society, 2019
The period of pulsation and the structure of the light curve for Cepheid and RR Lyrae variables depend on the fundamental parameters of the star: mass, radius, luminosity, and effective temperature.
Earl P. Bellinger   +3 more
openalex   +3 more sources

Benchmarking the fundamental parameters of Ap stars with optical long-baseline interferometric measurements [PDF]

open access: hybridAstronomy & Astrophysics, 2020
Context. The variety of physical processes at play in chemically peculiar stars makes it difficult to determine their fundamental parameters. In particular, for the magnetic ones, called Ap stars, the strong magnetic fields and the induced spotted ...
K. Perraut   +12 more
openalex   +2 more sources

Atmospheric and Fundamental Parameters of Eight Nearby Multiple Stars

open access: gold, 2022
We present the complete set of atmospheric and fundamental parameters, in addition to the masses, for the individual components of eight stellar systems.
Abdallah M. Hussein   +6 more
openalex   +2 more sources

Spectroscopic and physical parameters of Galactic O-type stars. II. Observational constraints on projected rotational and extra broadening velocities as a function of fundamental parameters and stellar evolution [PDF]

open access: green, 2013
Rotation is of key importance for the evolution of hot massive stars, however, the rotational velocities of these stars are difficult to determine. Based on our own data for 31 Galactic O stars and incorporating similar data for 86 OB supergiants from ...
N. Markova   +5 more
openalex   +3 more sources

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

open access: bronzeAstronomy & 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 ...
I. Karovicova   +13 more
openalex   +3 more sources

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