Galaxy Zoo: A sample of blue early-type galaxies at low redshift
| Autor: | Jan Vandenberg, Alexander S. Szalay, Chris Lintott, Kevin Schawinski, Dan Andreescu, M. Jordan Raddick, Sukyoung K. Yi, Robert C. Nichol, Kate Land, Phil Murray, Steven P. Bamford, Daniel Thomas, Sugata Kaviraj, Sadegh Khochfar, Anze Slosar, Marc Sarzi |
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| Jazyk: | angličtina |
| Rok vydání: | 2016 |
| Předmět: |
Physics
Cosmology and Gravitation education.field_of_study Cosmology and Nongalactic Astrophysics (astro-ph.CO) Star formation Metallicity Population FOS: Physical sciences Astronomy and Astrophysics Context (language use) Astrophysics::Cosmology and Extragalactic Astrophysics Astrophysics Galaxy Redshift Space and Planetary Science Galaxy formation and evolution Astrophysics::Solar and Stellar Astrophysics Emission spectrum education Astrophysics::Galaxy Astrophysics Astrophysics - Cosmology and Nongalactic Astrophysics |
| Zdroj: | Schawinski, K, Lintott, C J, Thomas, D, Sarzi, M, Andreescu, D, Bamford, S P, Kaviraj, S, Khochfar, S, Land, K, Murray, P, Nichol, R C, Raddick, M J, Slosar, A, Szalay, A, Vandenberg, J & Yi, S K 2009, ' Galaxy Zoo : a sample of blue early-type galaxies at low redshift ', Monthly Notices of the Royal Astronomical Society, vol. 396, no. 2, pp. 818-829 . https://doi.org/10.1111/j.1365-2966.2009.14793.x |
| Popis: | We report the discovery of a population of nearby, blue early-type galaxies with high star formation rates (0.5 < SFR < 50 Msun/yr). They are identified by their visual morphology as provided by Galaxy Zoo for SDSS DR6 and their u-r colour. We select a volume-limited sample in the redshift range 0.02 < z < 0.05, corresponding to luminosities of approximately L* and above, and with u-r colours significantly bluer than the red sequence. We confirm the early-type morphology of the objects in this sample and investigate their environmental dependence and star formation properties. Blue early-type galaxies tend to live in lower-density environments than `normal' red sequence early-types and make up 5.7 +/-0.4% of the low-redshift early-type galaxy population. We find that such blue early-type galaxies are virtually absent at high velocity dispersions above 200 km/s. Our analysis uses emission line diganostic diagrams and we find that ~25% of them are actively starforming, while another ~25% host both star formation and an AGN. Another ~12% are AGN. The remaining 38% show no strong emission lines. When present and uncontaminated by an AGN contribution, the star formation is generally intense. We consider star formation rates derived from Halpha, u-band and infrared luminosities, and radial colour profiles, and conclude that the star formation is spatially extended. Of those objects that are not currently undergoing star formation must have ceased doing so recently in order to account for their blue optical colours. The gas phase metallicity of the actively starforming blue early-types galaxies is supersolar in all cases. We discuss the place of these objects in the context of galaxy formation. A catalogue of all 204 blue early-type galaxies in our sample, including star formation rates and emission line classification, is provided. Accepted for publication in MNRAS. 18 pages, 14 figures, 2 tables. A version with full resolution figures is available at http://www.astro.yale.edu/ks57/papers/Schawinski.GZblueetypes.2009.pdf |
| Databáze: | OpenAIRE |
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