Molecular Hydrogen at high redshifts

Details Molecular Hydrogen at high redshifts Molecular Hydrogen at high redshifts

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002sf2a.conf..363p&link_type=abstract

SF2A-2002: Semaine de l'Astrophysique Francaise, meeting held in Paris, France, June 24-29, 2002, Eds.: F. Combes and D. Barret,

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present a survey for molecular hydrogen in damped Lyman-alpha systems
at redshift larger than 2. We show that presence of dust and high
particle density are necessary ingredient for the formation of
molecules. Properties of the gas are compared with what is measured in
the local ISM from FUSE observations.

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