Hostname: page-component-76fb5796d-vvkck Total loading time: 0 Render date: 2024-04-26T08:54:46.201Z Has data issue: false hasContentIssue false
  • English
  • Français

The Erupting Star in HD5980: A Rapid Rotator?

Published online by Cambridge University Press:  26 May 2016

Leonid Georgiev  and
Gloria Koenigsberger
Leonid Georgiev
Affiliation:
Instituto de Astronomía, UNAM, Mexico D.F., Mexico
Gloria Koenigsberger
Affiliation:
Centro de Ciencias Físicas, UNAM, Morelos, Mexico

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We present evidence suggesting that the star that erupted in 1994 in the SMC multiple system HD 5980 has v sin i ~230 km s–1, which is close to the breakup velocity for this star.

Type
Session 1 Observations of Rotating Stars
Information
Symposium - International Astronomical Union , Volume 215: Stellar Rotation , 2004 , pp. 111 - 112
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Koenigsberger, G., Moreno, E. 1999, RMAA 35, 157.Google Scholar
Koenigsberger, G., Kurucz, R., Georgiev, L., 2003, ApJ in press Google Scholar
Langer, N., 1997, ASP-CPS 120, p83 Google Scholar
Moffat, et al. 1998, ApJ 497, 896.Google Scholar
Niemela, V., Barba, R., Morrell, N., Corti, M., 1997, ASP-CPS 120, p220 Google Scholar