The 2dF Galaxy Redshift Survey: The environmental dependence of galaxy star formation rates near clusters

Mon.Not.Roy.Astron.Soc.334:673,2002 We have measured the equivalent width of the H-alpha emission line for 11006 galaxies brighter than M_b=-19 (LCDM) at 0.05

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Bibliographische Detailangaben
Hauptverfasser:	Lewis, Ian, Balogh, Michael, De Propris, Roberto, Couch, Warrick, Bower, Richard, Offer, Alison, Bland-Hawthorn, Joss, Baldry, Ivan, Baugh, Carlton, Bridges, Terry, Cannon, Russell, Cole, Shaun, Colless, Matthew, Collins, Chris, Cross, Nicholas, Dalton, Gavin, Driver, Simon, Efstathiou, George, Ellis, Richard, Frenk, Carlos, Glazebrook, Karl, Hawkins, Edward, Jackson, Carole, Lahav, Ofer, Lumsden, Stuart, Maddox, Steve, Madgwick, Darren, Norberg, Peder, Peacock, John, Percival, Will, Peterson, Bruce, Sutherland, Will, Taylor, Keith
Format:	Artikel
Sprache:	eng
Schlagworte:	Physics - Astrophysics of Galaxies Physics - Cosmology and Nongalactic Astrophysics Physics - Earth and Planetary Astrophysics Physics - High Energy Astrophysical Phenomena Physics - Instrumentation and Methods for Astrophysics Physics - Solar and Stellar Astrophysics
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Zusammenfassung:	Mon.Not.Roy.Astron.Soc.334:673,2002 We have measured the equivalent width of the H-alpha emission line for 11006 galaxies brighter than M_b=-19 (LCDM) at 0.05
DOI:	10.48550/arxiv.astro-ph/0203336