| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 9850967 | Nuclear Physics A | 2005 | 4 Pages |
Abstract
We present here the current status of both model predictions, from calculations of massive star evolution including rotation of stellar interior, and from data on γ2 Velorum obtained by the ESA's gamma-ray satellite INTEGRAL over the first year of its mission.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Nuclear and High Energy Physics
Authors
N. Mowlavi, J. Knödlseder, G. Meynet, P. Dubath, R. Diehl, G. Lichti, S. Schanne, C. Winkler,