Ultraviolet Spectropolarimetry: on the origin of rapidly rotating B stars-Reference-Cited by-同舟云学术

Ultraviolet Spectropolarimetry: on the origin of rapidly rotating B stars

Published:2022-12 Issue:12 Volume:367 Page:
ISSN:0004-640X
Container-title:Astrophysics and Space Science
language:en
Short-container-title:Astrophys Space Sci

Author:

Jones C. E.^ORCID,Labadie-Bartz J.,Cotton D. V.,Nazé Y.,Peters G. J.,Hillier D. J.,Neiner C.,Richardson N. D.,Hoffman J. L.,Carciofi A. C.,Wisniewski J. P.,Gayley K. G.,Suffak M. W.,Ignace R.,Scowen P. A.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://link.springer.com/content/pdf/10.1007/s10509-022-04127-5.pdf

Reference131 articles.

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2. Baade, D., Rivinius, T., Pigulski, A., et al.: Short-term variability and mass loss in Be stars. I. BRITE satellite photometry of $\eta$ and $\mu$ Centauri. Astron. Astrophys. 588, A56 (2016). https://doi.org/10.1051/0004-6361/201528026. arXiv:1602.01744 [astro-ph.SR]

3. Baade, D., Pigulski, A., Rivinius, T., et al.: Short-term variability and mass loss in Be stars. III. BRITE and SMEI satellite photometry of 28 Cygni. Astron. Astrophys. 610, A70 (2018). https://doi.org/10.1051/0004-6361/201731187. arXiv:1708.07360 [astro-ph.SR]

4. Bailey, J., Cotton, D.V., Howarth, I.D., et al.: The rotation of $\alpha$ Oph investigated using polarimetry. Mon. Not. R. Astron. Soc. 494(2), 2254–2267 (2020). https://doi.org/10.1093/mnras/staa785. arXiv:2003.07983 [astro-ph.SR]

5. Balona, L.A., Ozuyar, D.: TESS observations of Be stars: a new interpretation. Mon. Not. R. Astron. Soc. 493(2), 2528–2544 (2020). https://doi.org/10.1093/mnras/staa389. arXiv:1911.03068 [astro-ph.SR]

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