A new population of recently quenched elliptical galaxies in the SDSS

We use the Sloan Digital Sky Survey to investigate the properties of massive elliptical galaxies in the local Universe (z ≤ 0.08) that have unusually blue optical colours. Through careful inspection, we distinguish elliptical from non-elliptical morphologies among a large sample of similarly blue ga...

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Veröffentlicht in:Monthly notices of the Royal Astronomical Society 2014-07, Vol.442 (1), p.533-557
Hauptverfasser: McIntosh, Daniel H., Wagner, Cory, Cooper, Andrew, Bell, Eric F., Kereš, Dušan, Bosch, Frank C. van den, Gallazzi, Anna, Haines, Tim, Mann, Justin, Pasquali, Anna, Christian, Allison M.
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Sprache:eng
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Zusammenfassung:We use the Sloan Digital Sky Survey to investigate the properties of massive elliptical galaxies in the local Universe (z ≤ 0.08) that have unusually blue optical colours. Through careful inspection, we distinguish elliptical from non-elliptical morphologies among a large sample of similarly blue galaxies with high central light concentrations (c r  ≥ 2.6). These blue ellipticals comprise 3.7 per cent of all c r  ≥ 2.6 galaxies with stellar masses between 1010 and 1011 h −2 M⊙. Using published fibre spectrum diagnostics, we identify a unique subset of 172 non-star-forming ellipticals with distinctly blue urz colours and young (
ISSN:0035-8711
1365-2966
DOI:10.1093/mnras/stu808