Deep HST Imaging of Sextans A I. The Spatially Resolved Recent Star Formation History

Details Deep HST Imaging of Sextans A I. The Spatially Resolved Recent Star Formation History Deep HST Imaging of Sextans A I. The Spatially Resolved Recent Star Formation History

2001-10-10

arxiv.org/abs/astro-ph/0110257v1

Astron.J. 123 (2002) 813-831

Astronomy and Astrophysics

Astrophysics

27 pages, 14 figures, 2 mpeg movies, accepted in the Astronomical Journal

Scientific paper

10.1086/324635

We have measured stellar photometry from deep Cycle 7 Hubble Space Telescope/WFPC2 imaging of the dwarf irregular galaxy Sextans A. The imaging was taken in three filters: F555W ($V$; 8 orbits), F814W ($I$; 16 orbits), and F656N (H$\alpha$; 1 orbit). Combining these data with Cycle 5 WFPC2 observations provides nearly complete coverage of the optically visible portion of the galaxy. The Cycle 7 observations are nearly 2 magnitudes more sensitive than the Cycle 5 observations, which provides unambiguous separation of the faint blue helium burning stars (BHeB stars) from contaminant populations. The depth of the photometry allows us to compare recent star formation histories recovered from both the main sequence (MS) stars and the BHeB stars for the last 300 Myr. The excellent agreement between these independent star formation rate (SFR) calculations is a resounding confirmation for the legitimacy of using the BHeB stars to calculate the recent SFR. Using the BHeB stars we have calculated the global star formation history over the past 700 Myr. The history calculated from the Cycle 7 data is remarkably identical to that calculated from the Cycle 5 data, implying that both halves of the galaxy formed stars in concert. We have also calculated the spatially resolved star formation history, combining the fields from the Cycle 5 and Cycle 7 data. Our interpretation of the pattern of star formation is that it is an orderly stochastic process.

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