Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 432, Issue 1, Pages 430-437Publisher
OXFORD UNIV PRESS
DOI: 10.1093/mnras/stt478
Keywords
galaxies: elliptical and lenticular, cD; galaxies: formation; galaxies: photometry; galaxies: star formation; galaxies: stellar content; ultraviolet: galaxies
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Funding
- National Research Foundation (NRF)
- bilateral grant under the Indo-South Africa Science and Technology Cooperation [UID76354]
- Department of Science and Technology (DST) of the Indian Government
- Department of Science and Technology (DST) of the South African Government
- NASA
- Alfred P. Sloan Foundation
- National Science Foundation
- US Department of Energy Office of Science
- University of Arizona
- Brookhaven National Laboratory
- University of Cambridge
- Carnegie Mellon University
- University of Florida
- Harvard University
- Instituto de Astrofisica de Canarias
- Johns Hopkins University
- Lawrence Berkeley National Laboratory
- Max Planck Institute for Astrophysics
- Max Planck Institute for Extraterrestrial Physics
- New Mexico State University
- New York University
- Ohio State University
- Pennsylvania State University
- University of Portsmouth
- Princeton University
- University of Tokyo
- University of Utah
- Vanderbilt University
- University of Virginia
- University of Washington
- Yale University
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We combine UV/optical/near-IR/mid-IR data on a sample of similar to 240 S0 galaxies to examine various star formation related processes in them. We split the sample into bright and faint S0 galaxies based on their K-band luminosity. Comparing the far-ultraviolet (FUV)-near-ultraviolet (NUV) versus NUV-K colour-colour diagram with a simple stellar population model shows that ellipticals and bright S0 galaxies are dominated by a stellar population of age >10(9) yr while faint S0 galaxies may contain stars as young as 10(8) yr, providing evidence for relatively recent star formation activity. The strength of the 4000 angstrom break is also systematically higher in brighter S0 galaxies, again indicating the presence of an old stellar population. Their mid-IR colours indicate that bright S0 colours are like those of ellipticals while faint S0 colours are more like spirals. All these observations are consistent with a scenario in which low-luminosity S0 galaxies likely formed by the stripping of gas from the discs of late-type spiral galaxies, which in turn formed their pseudo-bulges through secular evolution processes, possibly involving multiple episodes of star formation. On the other hand, more luminous S0 galaxies likely formed the bulk of their stars at early epochs, similar to the star formation in elliptical galaxies, and are characterized by an old coeval stellar population and classical bulges.
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