HST/ACS observations of the old and metal-poor Sagittarius dwarf irregular galaxy

Details HST/ACS observations of the old and metal-poor Sagittarius dwarf irregular galaxy HST/ACS observations of the old and metal-poor Sagittarius dwarf irregular galaxy

2005-05-19

arxiv.org/abs/astro-ph/0505399v1

Astronomy and Astrophysics

Astrophysics

19 pages, 13 figures. Accepted for publication in A&A. A higher resolution version is available at ftp://ftp.pd.astro.it/pub/m

Scientific paper

10.1051/0004-6361:20052747

We have obtained deep color-magnitude diagrams of the Sagittarius dwarf irregular galaxy with the HST/ACS. The new diagrams unveil for the first time the star formation history of SagDIG. We identify a small population of red horizontal branch stars, which sets the first epoch of star formation in SagDIG back to ~9-10 Gyr ago. This shows that SagDIG has been able to maintain a very low mean metallicity (-2.2<[Fe/H]<-1.9) over a 10 Gyr life time, and most importantly, that all Local Group dwarf galaxies share an ancient (~10 Gyr) initial episode of star formation. Thus, at the moment, IZw18 remains the only exception to this general trend, favoring the so-called ``young galaxy'' scenario. However, a re-analysis of ACS observations of IZw18 suggests that an older RGB population may be present also in IZw18. We also compare the distribution of atomic hydrogen with that of stellar populations of various ages. We find little correlation between stellar populations older than ~1 Gyr and the HI. In particular we fail to find any generation of stars that preferentially lie within the large HI hole. We therefore exclude the possibility that the SagDIG ring-like HI distribution is the result of multiple supernova events. Alternative scenarios have to be explored.

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