V380 Cygni Once More: A Close Detached Binary with an Evolved B‐Type Component. I. Spectroscopic Orbits
Author:
Publisher
IOP Publishing
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/1538-3873/110/i=747/a=572/pdf
Reference16 articles.
1. The Atmospheres of the B Stars. V. The Spectrum of Gamma Pegasi.
2. Accurate masses and radii of normal stars
3. The apsidal motion of V 380 Cygni
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2. The eccentric massive binary V380 Cyg: revised orbital elements and interpretation of the intrinsic variability of the primary component*;Monthly Notices of the Royal Astronomical Society;2014-01-14
3. Detection of gravity modes in the massive binary V380 Cyg from Kepler space-based photometry and high-resolution spectroscopy★;Monthly Notices of the Royal Astronomical Society: Letters;2012-05-22
4. Chemical evolution of high-mass stars in close binaries ��� II. The evolved component of the eclipsing binary V380���Cygni;Monthly Notices of the Royal Astronomical Society;2009-12-01
5. Resolving stellar atmospheres;Astronomy & Astrophysics;2006-07-31
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