paper

The Outer Regions of the Nearby Sc Galaxies NGC 2403 and M33: Evidence for an Intermediate Age Population at Large Radii

arXiv:astro-ph/0304194 · doi:10.1086/375303

Abstract

Deep g'r'i'z' images obtained with the Gemini Multi-Object Spectrograph are used to investigate the stellar content in the outer regions of the nearby Sc galaxies NGC 2403 and M33. The red giant branch tip occurs at i' = 23.6 +/- 0.1 in NGC 2403, and the Cepheid and RGB-tip distance scales for this galaxy are in good agreement. While very young stars are restricted to radii < 10 kpc along the plane of the disk, a population of bright asymptotic giant branch (AGB) stars is present out to r = 20 kpc, indicating that star formation occured outside of the present-day star-forming disk of NGC 2403 during intermediate epochs. The AGB stars are not in a tidal stream; in fact, the ratio of AGB stars above the RGB-tip to those below the RGB-tip does not change with radius, indicating that the bright AGB stars are uniformly mixed with the fainter stellar content throughout the field. A similar population of bright AGB stars is detected in the outer regions of M33, and the ratio of bright AGB stars to stars on the upper RGB is at least as large as that measured in the outer regions of NGC 2403; thus, an intermediate-age population occurs well outside of the young star-forming disk of M33.

41 pages; 21 figures; to appear in AJ

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