Direct Observational Test Rules Out Small MgII Absorbers

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Accepted for publication in MNRAS Letters. 5 pages, 2 figures

Scientific paper

10.1111/j.1745-3933.2007.00377.x

Recent observations suggest the incidence of strong intervening MgII absorption systems along the line-of-sight to gamma ray burst (GRB) afterglows is significantly higher than expected from analogous quasar sightlines. One possible explanation is a geometric effect, arising because MgII absorbers only partially cover the quasar continuum regions, in which case MgII absorbers must be considerably smaller than previous estimates. We investigate the production of abnormal absorption profiles by partial coverage and conclude that the lack of any known anomalous profiles in observed systems, whilst constraining, cannot on its own rule out patchy MgII absorbers. In a separate test, we look for differences in the distribution function of MgII equivalent widths over quasar continuum regions and CIII] emission lines. We show that these anomalies should be observable in any scenario where MgII absorbers are very small, but they are not present in the data. We conclude that models invoking small MgII cloudlets to explain the excess of absorbers seen towards GRBs are ruled out.

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

Direct Observational Test Rules Out Small MgII Absorbers 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 Direct Observational Test Rules Out Small MgII Absorbers, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Direct Observational Test Rules Out Small MgII Absorbers will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-169701

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