On the significance of the excess number of strong Mg II absorbers observed toward gamma-ray bursts
The number of strong (equivalent width >1 Å) Mg II absorbers observed toward gamma-ray bursts (GRBs) has been found to be statistically larger than the number of strong absorbers toward quasi-stellar objects (QSOs). We formalize this "Mg II problem" and
|Collections||ANU Research Publications|
|Source:||Astrophysical Journal, The|
|01_Rapoport_On_the_significance_of_the_2013.pdf||1.59 MB||Adobe PDF|
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