Infalling Faint [OII] Emitters in Abell 851. II. Environment, Kinematics, and Star Formation History

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

23 pages (LaTeX emulateapj), 20 figures, to appear in ApJ. A version with high-resolution figures available from the lead auth

Scientific paper

10.1086/505567

We report on the environments, kinematics, and SFH of [OII]-selected objects in the z=0.4 galaxy cluster A851, using Keck optical spectra. A large fraction (~55%) of cluster [OII] emitters show strong Balmer absorptions (>4A in equivalent width at Hd). These e(a) spectra have been attributed to dusty starburst galaxies, an interpretation supported by our reddening measurements, which show a high frequency of very reddened [EBV>0.5] [OII] emitters. Our spectral modeling requires starburst ages >1Gyr, shorter than the cluster crossing timescale. We argue that this starburst phase occurs during cluster infall based on the radial velocity distribution of the cluster [OII] emitters, which present a deficit of systems near the cluster systemic velocity. The spatial segregation of some redshifted and blueshifted groups strongly indicates that the accretion was recent. Throughout the cluster, the fraction in [OII] emitters is a strong function of the local galaxy density. Our analysis supports previous suggestions that dusty starburst galaxies arise at the expense of gas-rich spiral galaxies. In addition, we describe a fainter [OII]-emitting population, comprised largely of dwarf galaxies and find an even stronger suppression of [OII] emission in high density environments among this subsample, indicative of more effective destruction by harassment and/or gas-stripping. Comparison to previous morphological studies, limited to the core of A851, suggests that galaxy-galaxy interactions may trigger the starbursts. The high e(a) galaxy fraction in A851 compared to that in the field, however, suggests that some cluster-specific mechanism, likely related to the dynamical assembly of the cluster, also contributes to the high number of starbursts. (abridged)

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Infalling Faint [OII] Emitters in Abell 851. II. Environment, Kinematics, and Star Formation History does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Infalling Faint [OII] Emitters in Abell 851. II. Environment, Kinematics, and Star Formation History, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Infalling Faint [OII] Emitters in Abell 851. II. Environment, Kinematics, and Star Formation History will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-184739

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.