Titlebook: Double Stars, Physical Properties and Generic Relations; Proceeding of IAU Co Bambang Hidayat,Zdeněk Kopal,Jürgen Rahe Conference proceedin

神刊

Malcontent

VV Orionis: A Well-Behaved Early-Type Eclipsing Binary System,mponent whose orbital period about the eclipsing pair is about 120 days. In recent years there have been several new photoelectric and spectroscopic investigations of this system, and the results of these are compared. Both the geometric and photometric orbital elements appear to be well determined.

Delirium

Wolf-Rayet Binaries: Evolutionary Causes for their Distribution in the Galaxy,4.In order to assess the relative importance of massive binary evolution as one of the ways to produce WR stars, the galactic distribution of WR binaries is compared with that of single WR stars using improved intrinsic parameters and new data for the fainter WR stars..In the galactic plane the incr