The massive binary HD 152218 revisited: A new colliding wind system in NGC 6231
Authors:
- H. SanaHSH. Sana
- Y. NazéYNY. Nazé
- B. O’donnellBOB. O’donnell
- G. RauwGRG. Rauw
- E. GossetEGE. Gosset
- 1 May 2008
- journal article
- Published by Elsevier in New Astronomy
- Vol. 13 (4) , 202-215
Abstract
No abstract availableKeywords
All Related Versions
This publication has 29 references indexed in Scilit:
- High-mass binaries in the very young open cluster NGC 6231Astronomy & Astrophysics, 2001
- $\vec{ UBVI}$ imaging photometry of NGC 6231Astronomy and Astrophysics Supplement Series, 1999
- CCD Strmgren Photometry of NGC 6231Monthly Notices of the Royal Astronomical Society, 1995
- On winds and X-rays of O-type starsThe Astrophysical Journal, 1991
- Approximations to the radii of Roche lobesThe Astrophysical Journal, 1983
- A survey of interstellar H I from L-alpha absorption measurements. IIThe Astrophysical Journal, 1978
- Spectroscopic studies of O-type stars. VIII - Radial velocities and the K-termThe Astrophysical Journal, 1977
- Spectroscopic studies of O-type stars. III. The effective temperature scale.The Astrophysical Journal, 1973
- Spectroscopic studies of O-type stars. II. Comparison with non-LTE models.The Astrophysical Journal, 1973
- Spectroscopic Studies of O-Type Stars. I. Classification and Absolute MagnitudesThe Astrophysical Journal, 1971