Chemical Composition of RM_1-390 - Large Magellanic Cloud Red Supergiant
نویسندگان
چکیده
منابع مشابه
Chemical Evolution in the Large Magellanic Cloud
We present a new input parameter set of the Pagel model for the LMC (Pagel & Tautvaĭsienė 1998) in order to reproduce the observations, including the star formation rate (SFR) history. It is concluded that high ratio of A (∼ 0.17), which is the probability for 3-8M stars to explode as SNe Ia, is required. As a result, a steep initial mass function (IMF) slope or existence of the outflow is not ...
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ژورنال
عنوان ژورنال: Journal of Astronomy and Space Sciences
سال: 2017
ISSN: 2093-5587
DOI: 10.5140/jass.2017.34.3.199