Astronomy and Astrophysics – Astrophysics
Scientific paper
1998-04-24
Astronomy and Astrophysics
Astrophysics
8 pages, To appear in Proceedings of the Workshop on H_2 in the Early Universe, eds. F. Palla, E. Corbelli, and D. Galli, Memo
Scientific paper
Molecules dominate the cooling function of neutral metal-poor gas at high density. Observation of molecules at high redshift is thus an important tool toward understanding the physical conditions prevailing in collapsing gas. Up to now, detections are sparse because of small filling factor and/or sensitivity limitations. However, we are at an exciting time where new capabilities offer the propect of a systematic search either in absorption using the UV Lyman-Werner H2 bands or in emission using the CO emission lines redshifted in the sub-millimeter.
No associations
LandOfFree
Molecules in QSOs and QSO Absorption Line Systems at High Redshift 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 Molecules in QSOs and QSO Absorption Line Systems at High Redshift, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Molecules in QSOs and QSO Absorption Line Systems at High Redshift will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-125853