MgII absorbers embedded in the 1040+05 quasar supercluster

Details MgII absorbers embedded in the 1040+05 quasar supercluster MgII absorbers embedded in the 1040+05 quasar supercluster

May 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aas...194.8703w&link_type=abstract

American Astronomical Society, 194th AAS Meeting, #87.03; Bulletin of the American Astronomical Society, Vol. 31, p.979

Statistics

Scientific paper

The largest structure known at z>0.2 consists of a large group of at least 15 quasars at 1.211.2 distributed over a ~ 2(deg) area embedded in the quasar group toward ESO/SERC field 927. Statistics for the redshift distribution of MgII absorbers with rest equivalent width W_0(lambda 2796) >= 0.3 Angstroms established by Steidel & Sargent et al. (1992, ApJS 80, 1 ) are used for comparison, and degree-wide structures are searched and compared with similar surveys at z>2 through CIV absorbers (Williger et al. 1996, ApJS 104, 145). Our current results are presented and discussed.

Affiliated with

Also associated with

No associations

Rating

MgII absorbers embedded in the 1040+05 quasar supercluster 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 MgII absorbers embedded in the 1040+05 quasar supercluster, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and MgII absorbers embedded in the 1040+05 quasar supercluster will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1122256