DISCOVERY OF THE FIRST B[e] SUPERGIANTS IN M 31

B[e] supergiants (B[e]SGs) are transitional objects in the post-main sequence evolution of massive stars. The small number of B[e]SGs known so far in the Galaxy and the Magellanic Clouds indicates that this evolutionary phase is short. Nevertheless, the strong aspherical mass loss occurring during t...

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Veröffentlicht in:	Astrophysical journal. Letters 2014-01, Vol.780 (1), p.1-5
Hauptverfasser:	Kraus, M, Cidale, L S, Arias, M L, Oksala, M E, Fernandes, Borges M
Format:	Artikel
Sprache:	eng
Schlagworte:	ASTROPHYSICS ASTROPHYSICS, COSMOLOGY AND ASTRONOMY CARBON MONOXIDE Chemical evolution Classification COLOR Diagnostic systems Evolutionary GALACTIC EVOLUTION MAGELLANIC CLOUDS MASS TRANSFER Massive stars METALLICITY Progenitors (astrophysics) RESOLUTION Similarity STAR EVOLUTION Stars STELLAR WINDS SUPERGIANT STARS SUPERNOVAE
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