Improved estimates of the physical properties of the O-star binary V1007 Sco = HD 152248 and notes on several other binaries in the NGC 6231 cluster-Reference-Cited by-同舟云学术

Improved estimates of the physical properties of the O-star binary V1007 Sco = HD 152248 and notes on several other binaries in the NGC 6231 cluster

Published:2008-01-25 Issue:1 Volume:481 Page:183-192
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Mayer P.,Harmanec P.,Nesslinger S.,Lorenz R.,Drechsel H.,Morrell N.,Wolf M.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361:20078542/pdf

Reference55 articles.

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3. $\vec{ UBVI}$ imaging photometry of NGC 6231

4. Bouzid, M. Y., & Sterken, C. 2004, in Spectroscopically and Spatially Resolving the Components of the Close Binary Stars, ed. R. W. Hilditch, H. Hensberge, & K. Pavlovski, ASP Conf. Ser., 318, 288

5. Photoelectric Magnitudes and Colors in NGC 6231.

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