Astronomy and Astrophysics – Astrophysics
Scientific paper
2004-10-27
Astrophys.J. 620 (2005) L795
Astronomy and Astrophysics
Astrophysics
5 pages, 3 figures To be published in the Astrophysical Journal
Scientific paper
10.1086/427164
Recent observations suggest that the behaviour of tracer species such as N_2H+ and CS is significantly different in regions of high and low mass star formation. In the latter, N_2H+ is a good tracer of mass, while CS is not. Observations show the reverse to be true in high-mass star formation regions. We use a computational chemical model to show that the abundances of these and other species may be significantly altered by a period of accelerated collapse in high mass star forming regions. We suggest these results provide a potential explanation of the observations, and make predictions for the behaviour of other species.
Caselli Paola
Hartquist Thomas W.
Lintott Chris J.
Myers Philip
Rawlings Jonathan M. C.
No associations
LandOfFree
Molecular abundance ratios as a tracer of accelerated collapse in regions of high mass star formation? 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 Molecular abundance ratios as a tracer of accelerated collapse in regions of high mass star formation?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Molecular abundance ratios as a tracer of accelerated collapse in regions of high mass star formation? will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-341754