A spectroscopic investigation of the O-type star population in four Cygnus OB associations
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361/201321985/pdf
Reference58 articles.
1. Collective pulsational velocity broadening due to gravity modes as a physical explanation for macroturbulence in hot massive stars
2. Lower mass loss rates in O-type stars: Spectral signatures of dense clumps in the wind of two Galactic O4 stars
3. Properties of Galactic early-type O-supergiants
4. Rotating massive main-sequence stars
5. Rotating massive main-sequence stars
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