An Age Estimate for the NGC456, 460 and 465 SMC Constellation
Part of the Astrophysics and Space Science Library book series (ASSL, volume 155)
The aim of this paper is to study the distribution of spectral types of the stellar content in an outlying region (wing) of the Small Magellanic Cloud (SMC) which contains the brightest early type stars and therefore the most massive in this galaxy.
KeywordsSpectral Type Type Star Late Type Star Spectral Classification Small Magellanic Cloud
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.
© Kluwer Academic Publisher 1989