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- W2895842028 abstract "Abstract We analysed a population of bright-red (BR) stars in the dwarf irregular galaxy Leo A by using multicolour photometry data obtained with the Subaru/Suprime-Cam ( B , V , R , I , Hα ) and HST/ACS ( F 475 W & F 814 W ) instruments. In order to separate the Milky Way (MW) and Leo A populations of red stars, we developed a photometric method, which enabled us to study the spatial distribution of BR stars within the Leo A galaxy. We found a significant difference in the scale-length (S-L) of radial distributions of the “young” and “old” red giant branch (RGB) stars – 0′.82 ± 0′.04 and 1′53 ± 0′.03, respectively. Also, we determined the S-L of BR stars of 0′.85 ± 0′.05, which closely matches that of the “young” RGB stars. Additionally, we found a sequence of peculiar RGB stars and 8 dust-enshrouded stars in the Leo A galaxy." @default.
- W2895842028 created "2018-10-26" @default.
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- W2895842028 date "2018-08-01" @default.
- W2895842028 modified "2023-09-23" @default.
- W2895842028 title "Bright-red stars in the dwarf irregular galaxy Leo A" @default.
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- W2895842028 doi "https://doi.org/10.1017/s1743921318006427" @default.
- W2895842028 hasPublicationYear "2018" @default.
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