First results from the Goddard High-Resolution Spectrograph - Evidence for photospheric microturbulence in early O stars - Are surface gravities systematically underestimated?
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Cited by 22 articles. 订阅此论文施引文献 订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献
1. Stellar wind properties of the nearly complete sample of O stars in the low metallicity young star cluster NGC 346 in the SMC galaxy;Astronomy & Astrophysics;2022-10
2. On the consistent treatment of the quasi-hydrostatic layers in hot star atmospheres;Astronomy & Astrophysics;2015-04-23
3. A BAKE-OFF BETWEEN CMFGEN AND FASTWIND: MODELING THE PHYSICAL PROPERTIES OF SMC AND LMC O-TYPE STARS;The Astrophysical Journal;2013-04-09
4. Sub-surface convection zones in hot massive stars and their observable consequences;Astronomy & Astrophysics;2009-03-12
5. On the role of ‘two-particle-one-hole’ resonances in electron collisions with Ni V;Journal of Physics B: Atomic, Molecular and Optical Physics;2005-12-19
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