神刊
发表于 2025-4-1 02:04:08
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Malcontent
发表于 2025-4-1 08:16:38
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
发表于 2025-4-1 10:21:42
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