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...
Autor Principal: | Vivas A. Katherina |
---|---|
Formato: | Artigo |
Idioma: | English |
Publicado: |
EDP Sciences
2017-01-01
|
Series: | EPJ Web of Conferences |
Acceso en liña: | https://doi.org/10.1051/epjconf/201715202008 |
Títulos similares
-
A Search for Faint Resolved Galaxies Beyond the Milky Way in DES Year 6: A New Faint, Diffuse Dwarf Satellite of NGC 55
por: M. McNanna, et al.
Publicado: (2024-01-01) -
Gas and Star Formation in Satellites of Milky Way Analogs
por: Michael G. Jones, et al.
Publicado: (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
por: Seungsoo Hong, et al.
Publicado: (2024-01-01) -
Catalogue of variable stars in Milky Way globular clusters
por: Clement Christine
Publicado: (2017-01-01) -
PORTRAIT OF A DARK HORSE: A PHOTOMETRIC AND SPECTROSCOPIC STUDY OF THE ULTRA-FAINT MILKY WAY SATELLITE PEGASUS III
por: Kim, Dongwon, et al.
Publicado: (2017)