Fe II emission lines in Be stars-Reference-Cited by-同舟云学术

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Fe II emission lines in Be stars

Published:2006-09-12 Issue:3 Volume:460 Page:821-829
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Arias M. L.,Zorec J.,Cidale L.,Ringuelet A. E.,Morrell N. I.,Ballereau D.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361:20065160/pdf

Reference55 articles.

1. Arias, M. L. 2004, Ph.D. Thesis, University of La Plata, Argentina

2. Arias, M. L., Zorec, J., Frémat, Y. 2006, In Active OB-Stars: laboratories for stellar and circumstellar physics, in press

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1. Spectroscopic study of Herbig Ae/Be stars in the Galactic anti-centre region from LAMOST DR5;Monthly Notices of the Royal Astronomical Society;2023-07-13

2. A stripped-companion origin for Be stars: clues from the putative black holes HR 6819 and LB-1;Monthly Notices of the Royal Astronomical Society;2021-02-03

3. Optical spectroscopy of Galactic field classical Be stars;Monthly Notices of the Royal Astronomical Society;2020-11-10

4. Be and Bn stars: Balmer discontinuity and stellar-class relationship;Astronomy & Astrophysics;2020-01-30

5. Spectral Classification and Estimation of Distances to the Be/X-Ray Binaries 1H1936+541 and 1H2202+501;Kinematics and Physics of Celestial Bodies;2019-01

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