Faint (and bright) variable stars in the satellites of the Milky Way
I describe two ongoing projects related with variable stars in the satellites of the MilkyWay. In the first project, we are searching for dwarf Cepheid stars (a.k.a δ Scuti and/or SX Phe) in some of the classical dwarf spheroidal galaxies. Our goal is to characterize the population of these variable...
Κύριος συγγραφέας: | Vivas A. Katherina |
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Μορφή: | Άρθρο |
Γλώσσα: | English |
Έκδοση: |
EDP Sciences
2017-01-01
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Σειρά: | EPJ Web of Conferences |
Διαθέσιμο Online: | https://doi.org/10.1051/epjconf/201715202008 |
Παρόμοια τεκμήρια
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A Search for Faint Resolved Galaxies Beyond the Milky Way in DES Year 6: A New Faint, Diffuse Dwarf Satellite of NGC 55
ανά: M. McNanna, κ.ά.
Έκδοση: (2024-01-01) -
Gas and Star Formation in Satellites of Milky Way Analogs
ανά: Michael G. Jones, κ.ά.
Έκδοση: (2024-01-01) -
Comparison of the Chemical Compositions between the Bright and Faint Red Clumps for the Metal-poor and Metal-rich Populations in the Milky Way Bulge
ανά: Seungsoo Hong, κ.ά.
Έκδοση: (2024-01-01) -
Catalogue of variable stars in Milky Way globular clusters
ανά: Clement Christine
Έκδοση: (2017-01-01) -
PORTRAIT OF A DARK HORSE: A PHOTOMETRIC AND SPECTROSCOPIC STUDY OF THE ULTRA-FAINT MILKY WAY SATELLITE PEGASUS III
ανά: Kim, Dongwon, κ.ά.
Έκδοση: (2017)