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- W3100294988 abstract "The stellar density distribution of the bulge is analyzed through one of its tracers. We use oxygen-rich Mira variables from the Catchpole et al. survey and OGLE-III survey as standard candles. The average age of these stars is around 9 Gyr. The population traced by Mira variables matches a boxy bulge prediction, not an X-shaped one, because only one peak is observed in the density along the analyzed lines of sight, whereas the prediction of an X-shape gives two clear peaks." @default.
- W3100294988 created "2020-11-23" @default.
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- W3100294988 date "2017-02-22" @default.
- W3100294988 modified "2023-09-27" @default.
- W3100294988 title "Absence of an X-shaped Structure in the Milky Way Bulge Using Mira Variable Stars" @default.
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- W3100294988 doi "https://doi.org/10.3847/1538-4357/836/2/218" @default.
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