Fragmentation and Collapse in Coronae-Australis

Details Fragmentation and Collapse in Coronae-Australis Fragmentation and Collapse in Coronae-Australis

Jul 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981mnras.196p..29l&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Vol. 196, P. 29P, 1981

Astronomy and Astrophysics

Astronomy

7

Scientific paper

Observations of H I in the vicinity of the dust lane of Corona Austrinae reveal a region of almost complete conversion of H I to H2. The results suggest that about 103Msun of material may be in a state of collapse. The projected centre of this region coincides with a small dense cloud which may be the physical centre of the collapsing fragment, while the limits of the collapsing zone appear to be defined by an almost complete dust ring of diameter 1.3 pc.

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