LEADER 01805nam  2200349z- 450 
001 9910557287203321
005 20231214133139.0
035   $a(CKB)5400000000041168
035   $a(oapen)https://directory.doabooks.org/handle/20.500.12854/68825
035   $a(EXLCZ)995400000000041168
100   $a20202105d2020      |y             0
101 0 $aeng
135   $aurmn|---annan
181   $ctxt$2rdacontent
182   $cc$2rdamedia
183   $acr$2rdacarrier
200 10$aLuminous Stars in Nearby Galaxies
210   $aBasel, Switzerland$cMDPI - Multidisciplinary Digital Publishing Institute$d2020
215   $a1 electronic resource (212 p.)
311   $a3-03936-280-1 
311   $a3-03936-281-X 
330   $aStudies 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.
606   $aResearch & information: general$2bicssc
606   $aAstronomy, space & time$2bicssc
615  7$aResearch & information: general
615  7$aAstronomy, space & time
700   $aHumphreys$b Roberta M$4edt$01281269
702   $aHumphreys$b Roberta M$4oth
906   $aBOOK
912   $a9910557287203321
996   $aLuminous Stars in Nearby Galaxies$93018446
997   $aUNINA