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

Lewis, I.; Balogh, M.; Propris, R. De; Couch, W.; Bower, R.; Offer, A.; Bland-Hawthorn, J.; Baldry, I. K.; Baugh, C.; Bridges, T.; Cannon, R.; Cole, S.; Colless, M.; Collins, C.; Cross, N.; Dalton, G.; Driver, S. P.; Efstathiou, G.; Ellis, R. S.; Frenk, C. S.; Glazebrook, K.; Hawkins, E.; Jackson, C.; Lahav, O.; Lumsden, S.; Maddox, S.; Madgwick, D.; Norberg, P.; Peacock, J. A.; Percival, W.; Peterson, B. A.; Sutherland, W.; Taylor, K.

doi:10.1046/j.1365-8711.2002.05558.x

articleMonthly Notices of the Royal Astronomical SocietyAug 11, 2002BRONZE OA

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

ILI. LewisMBM. BaloghRDR. De ProprisWCW. CouchRBR. Bower

Australian Astronomical Observatory · UNSW Sydney · +12 more institutions

Indexed inarxivcrossrefdoaj

Abstract

We have measured the equivalent width of the Hα emission line for 11 006 galaxies brighter than Mb=−19 (ΩΛ= 0.7, Ωm= 0.3, H0= 70 km s−1 Mpc−1) at 0.05

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Authors

33

IL
I. LewisCorresponding
Australian Astronomical Observatory
MB
M. Balogh
RD
R. De Propris
UNSW Sydney
WC
W. Couch
UNSW Sydney
RB
R. Bower
Durham University

Topics & keywords

Topics

Keywords

Velocity dispersion
Galaxy
Star formation
Virial mass
Virial theorem
Galaxy cluster
Brightest cluster galaxy
Redshift

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