SIMBAD references

2008MNRAS.388.1152P - Mon. Not. R. Astron. Soc., 388, 1152-1160 (2008/August-2)

Star formation in galaxies falling into clusters along supercluster-scale filaments.

PORTER S.C., RAYCHAUDHURY S., PIMBBLET K.A. and DRINKWATER M.J.

Abstract (from CDS):

With the help of a statistical parameter derived from optical spectra, we show that the current star formation rate of a galaxy, falling into a cluster along a supercluster filament, is likely to undergo a sudden enhancement before the galaxy reaches the virial radius of the cluster. From a sample of 52 supercluster-scale filaments of galaxies joining a pair of rich clusters of galaxies within the two-degree Field Redshift Survey region, we find a significant enhancement of star formation, within a narrow range between ∼2 and 3h–170 Mpc of the centre of the cluster into which the galaxy is falling. This burst of star formation is almost exclusively seen in the fainter dwarf galaxies (MB≥ -20). The relative position of the peak does not depend on whether the galaxy is a member of a group or not, but non-group galaxies have on average a higher rate of star formation immediately before falling into a cluster. From the various trends, we conclude that the predominant process responsible for this rapid burst is the close interaction with other galaxies falling into the cluster along the same filament, if the interaction occurs before the gas reservoir of the galaxy gets stripped off due to the interaction with the intracluster medium.

Abstract Copyright: © 2008 The Authors. Journal compilation © 2008 RAS

Journal keyword(s): galaxies: clusters: general - galaxies: evolution - galaxies: starburst - cosmology: observations - large-scale structure of Universe

Simbad objects: 85

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2008MNRAS.388.1152P and select 'bookmark this link' or equivalent in the popup menu


2019.12.10-01:45:36

© Université de Strasbourg/CNRS

    • Contact