Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

High-resolution images of the Orion molecular ridge in the CS J = 2-1 transition

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/166010· OSTI ID:7222456
A maximum entropy algorithm is used to combine various data in order to obtain 7.5-arcsec resolution images of the CS J = 2-1 emission from a 3.5-arcmin section of the Orion molecular ridge. This section of the ridge is found to contain four condensations with nearly thermal CS peak brightness temperatures, dimensions from 0.03-0.11 pc, and virial masses from 30-80 solar masses. About 70 percent of the total mass within the 3-arcmin region is shown to be contained in these condensations. It is suggested that the condensations and the included section of the ridge form a gravitationally bound subunit of the Orion cloud. 27 references.
Research Organization:
Owens Valley Radio Observatory, Pasadena, CA (USA); National Radio Astronomy Observatory, Socorro, NM (USA); Onsala Rymdobservatorium (Sweden)
OSTI ID:
7222456
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 325; ISSN ASJOA
Country of Publication:
United States
Language:
English

Similar Records

Protostellar condensations within the Orion ridge
Journal Article · Thu May 01 00:00:00 EDT 1986 · Astrophys. J.; (United States) · OSTI ID:5266694

C-13O in Orion
Journal Article · Mon Mar 31 23:00:00 EST 1986 · Astrophys. J.; (United States) · OSTI ID:5429120

High spatial resolution observations of Orion bright bar: CS (J = 1-0) and H51. cap alpha. emission
Journal Article · Sun Jul 15 00:00:00 EDT 1984 · Astrophys. J., Lett. Ed.; (United States) · OSTI ID:6442360