Titlebook: Evolution of Massive Stars; A Confrontation betw D. Vanbeveren,W. Rensbergen,C. Loore Book 1994 Springer Science+Business Media Dordrecht 1

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Grasping

mendacity

LTE and NLTE Abundances in A-Supergiants a Test of Their Evolutionary Statuses between the scenarios depend on the input assumptions for several physical parameters, ., treatments for convection parameters and mass loss rates. A review of the predictions of evolution calculations for 10–30 solar mass stars is given by Fitzpatrick & Garmany (1991).

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https://doi.org/10.1007/978-94-011-1080-8Galaxy; Population; Supernova; astrophysics; galaxies; milky way; photometry; spectroscopy; star; stellar; ste

lymphedema

978-94-010-4471-4Springer Science+Business Media Dordrecht 1994

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難理解

overwrought

https://doi.org/10.1007/978-3-322-82282-6f 30 Doradus in the Large Magellanic Cloud (LMC). Using photometric data for over 2400 stars (complete to .≈ 18 mag), and spectroscopic observations of over 150 stars in the region, the best estimate of the initial mass function (IMF) yields a slope of Г = ?1.5 ± 0.2 for masses > 12.⊙, where the Sal

MUMP

https://doi.org/10.1007/978-3-322-91326-5le is known about the Be star content of the Magellanic Clouds (MCs). We present a refined method of Be star identification by CCD photometry and apply it to four young clusters and associations in the MCs. We find NGC 330 in the SMC to be exceptionally rich in Be stars, while the fraction is clearl

Rodent

Erfolg mit konsistenten Partnernic goal of studying the upper end of the stellar mass function at ultraviolet wavelengths where the color degeneracy encountered in visual CMDs is less severe. The CMD has been compared to a set of theoretical isochrones, which have been computed using the latest generation of evolutionary models an