Chemical Composition of RM_1-390 - Large Magellanic Cloud Red Supergiant

A high resolution spectroscopic observation of the red supergiant star RM_1-390 in the Large Magellanic Cloud was made from a 3.6 m telescope at the European Southern Observatory. Spectral resolving power was R=20,000, with a signal-to-noise ratio S/N > 100. We found the atmospheric parameters of...

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Autors principals:	Alexander V. Yushchenko, Yeuncheol Jeong, Vira F. Gopka, Svetlana V. Vasil’eva, Sergey M. Andrievsky, Volodymyr O. Yushchenko
Format:	Artigo
Idioma:	Inglês
Publicat:	The Korean Space Science Society 2017-09-01
Col·lecció:	Journal of Astronomy and Space Sciences
Matèries:	supergiants (RM_1-390) individual (RM_1-390) abundances accretion chemically peculiar
Accés en línia:	http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2017/v34n3/OJOOBS_2017_v34n3_199.pdf
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