Fourier analysis of He 4471/Mg 4481 line profiles for separating rotational velocity and axial inclination in rapidly rotating B-type stars-Reference-Cited by-同舟云学术

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Fourier analysis of He 4471/Mg 4481 line profiles for separating rotational velocity and axial inclination in rapidly rotating B-type stars

Published:2017-08-05 Issue:1 Volume:472 Page:230-244
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Takeda Y.^ORCID,Kawanomoto S.,Ohishi N.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/472/1/230/19679188/stx2021.pdf

Reference40 articles.

1. Rotational Velocities of B Stars

2. Analyses of Light Ion Spectra in Stellar Atmospheres.IV. H II in the B Stars

3. The Broadening of He I lines including ion dynamic corrections, with application to λ4471Å

4. Comprehensive tables for the interpretation and modeling of the light curves of eclipsing binaries

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1. ZPEKTR: A code for spectral synthesis of fast-rotating stars;Astronomy & Astrophysics;2024-05

2. Properties of the Be-type stars in 30 Doradus;Monthly Notices of the Royal Astronomical Society;2022-03-09

3. On the rotational velocity of Sirius A;Monthly Notices of the Royal Astronomical Society;2020-09-19

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