Predicted observational effects of rapid rotation for Be stars
- 30 October 2025
- journal article
- research article
- Published by Springer Nature in Astrophysics and Space Science
- Vol. 370 (10) , 1-24
Abstract
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Funding Information
- Natural Sciences and Engineering Research Council of Canada (Postgraduate scholarship--Doctoral, Discovery Grant)
- European Union (ERC, MAGNIFY, Project 101126182)
- NASA, Chandra Award (TM4-25001A)
- Conselho Nacional de Desenvolvimento Científico e Tecnológico (grant 314545/2023-9)
- São Paulo Research Foundation (grants 2018/04055-8 and 2019/13354-1)
This publication has 51 references indexed in Scilit:
- Transport of angular momentum by stochastically excited waves as an explanation for the outburst of the rapidly rotating Be star HD49330Astronomy & Astrophysics, 2020
- Investigating the lack of main-sequence companions to massive Be starsAstronomy & Astrophysics, 2020
- Critical study of the distribution of rotational velocities of Be starsAstronomy & Astrophysics, 2016
- Multitechnique testing of the viscous decretion disk modelAstronomy & Astrophysics, 2015
- Classical Be starsThe Astronomy and Astrophysics Review, 2013
- Gravity darkening in rotating starsAstronomy & Astrophysics, 2011
- The circumstellar discs of Be starsProceedings of the International Astronomical Union, 2010
- Stellar Atmospheres: Theory and Observations1997
- Infrared observations of Be stars from 2,3 to 19,5 microns.The Astrophysical Journal, 1974
- Theoretical H-Beta Line Profiles and Related Parameters for Rotating B StarsThe Astrophysical Journal, 1966