Luminous Stars in Nearby Galaxies

Studies on the populations of luminous stars in nearby resolved galaxies have revealed a complex distribution in the luminosity-temperature plane (the HR diagram). The fundamentals of massive star evolution are mostly understood, but the roles of mass loss, episodic mass loss, rotation, and binarity...

Full description

Saved in:
Bibliographic Details
Other Authors: Humphreys, Roberta M. (Editor)
Format: Electronic Book Chapter
Language:English
Published: Basel, Switzerland MDPI - Multidisciplinary Digital Publishing Institute 2020
Subjects:
Online Access:DOAB: download the publication
DOAB: description of the publication
Tags: Add Tag
No Tags, Be the first to tag this record!
Description
Summary:Studies on the populations of luminous stars in nearby resolved galaxies have revealed a complex distribution in the luminosity-temperature plane (the HR diagram). The fundamentals of massive star evolution are mostly understood, but the roles of mass loss, episodic mass loss, rotation, and binarity are still in question. Moreover, the final stages of these stars of different masses and their possible relation to each other are not understood. The purpose of this volume is to provide a current review of the different populations of evolved massive stars. The emphasis is on massive stars in the Local Group, the Magellanic Clouds, and the nearby spirals M31 and M33.
Physical Description:1 electronic resource (212 p.)
ISBN:books978-3-03936-281-3
9783039362806
9783039362813
Access:Open Access