Local Cosmology from Isolated Dwarfs: variable stars from the LCID project.

Bibcode
2008MmSAI..79..732M
Monelli, M.; Bernard, E.; LCID Team
Bibliographical reference

Memorie della Società Astronomica Italiana, v.79, p.732 (2008)

Advertised on:
0
2008
Number of authors
3
IAC number of authors
1
Citations
0
Refereed citations
0
Description
During Cycle 14 a total of 113 HST orbits were secured to observe five isolated dwarf galaxies, namely Tucana, LGS3, LeoA, IC1613, and Cetus. The aim of the project is a full characterization of the stellar content of these galaxies, in terms of their SFH, radial distributions, halo populations and variable stars. Deep (V≈29) F475W, F814W data allowed us to fully sample all the evolutionary phases from the tip of the Red Giant Branch (RGB) to well below the old Main Sequence Turnoff (MSTO). Here we briefly summarize the latest results of the LCID project concerning the variable star content of our sample galaxies.
Type
Non-refereed
Galaxies
Photometry
Techniques

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