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Subaru Hyper Suprime-Cam Survey for the Local Group Dwarf Galaxies: Ursa Minor

Published online by Cambridge University Press:  30 October 2019

Yutaka Komiyama*
Affiliation:
National Astronomical Observatory of Japan, 2-21-1, Osawa, Mitaka, Tokyo 181-8588, Japan, email: komiyama@subaru.naoj.org
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Abstract

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We have carried out a wide and deep imaging survey for the Local Group dwarf spheroidal galaxy Ursa Minor (UMi) using Hyper Suprime-Cam (HSC). The data cover out beyond the nominal tidal radius down to ~25 mag in i band, which is ~2 mag below the main sequence turn-off point. The structural parameters of UMi are derived using red giant branch (RGB) stars and sub-giant branch (SGB) stars, and the tidal radius is suggested to be larger than those estimated by the previous studies. It is also found that the distribution of bluer RGB/SGB stars is more extended than that of redder RGB/SGB stars. The fraction of binary systems is estimated to be ~0.4 from the morphology of the main sequences.

Type
Contributed Papers
Copyright
© International Astronomical Union 2019 

References

Irwin, M. J., & Hatzidimitriou, D. 1995, MNRAS, 277, 1354 CrossRefGoogle Scholar
Kleyna, J. T., Geller, M. J., & Kenyon, S. J. et al. 1995, AJ, 115, 2359 CrossRefGoogle Scholar
Milone, A. P., Piotto, G., King, & I. R. et al. 2010, ApJ, 709, 1183 CrossRefGoogle Scholar
Minor, Q. E. 2013, ApJ, 779, 116 CrossRefGoogle Scholar
Palma, C., Majewski, S. R., & Siegel, M. H. et al. 2003, AJ, 125, 1352 CrossRefGoogle Scholar
Solima, A, Beccari, G., & Ferraro, F. R. et al. 2007, MNRAS, 380, 781 CrossRefGoogle Scholar