Low Mass Star Formation in the Norma Cloud

Details Low Mass Star Formation in the Norma Cloud Low Mass Star Formation in the Norma Cloud

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008hsf2.book..381r&link_type=abstract

Handbook of Star Forming Regions, Volume II: The Southern Sky ASP Monograph Publications, Vol. 5. Edited by Bo Reipurth, p.381

Computer Science

Scientific paper

A small filamentary cloud in Norma hosts a number of young low-mass stars in various stages of evolution, from visible Hα emission stars to embedded sources detected only in the sub-millimeter regime. The best known source is V346 Nor, an FU Orionis star that brightened in the early 1980s. The morphology of the cloud complex and an apparent age gradient along the cloud suggests that star formation in this region was triggered by an external event.

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