High-resolution CO observations of young low-mass stars

Details High-resolution CO observations of young low-mass stars High-resolution CO observations of young low-mass stars

May 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...340..472t&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 340, May 1, 1989, p. 472-478.

Astronomy and Astrophysics

Astronomy

97

Carbon Monoxide, Early Stars, Molecular Clouds, Stellar Mass, Stellar Mass Accretion, High Resolution, Infrared Astronomy Satellite, Interferometry, Star Formation

Scientific paper

Through the use of the Owens Valley Millimeter Interferometer, CO(1-0) emission near very young low-mass stars was observed. The data consist of a snapshot visibility survey of 25 low-luminosity IRAS sources associated with dense molecular cores and full aperture synthesis maps of two cores, L1262 and L1681B. The two sources mapped show spatially compact low-velocity outflows. The momentum flux in the compact outflows is comparable to that powering larger scale low-luminosity outflows. Extrapolating from the results of the snapshot survey, at least 64 percent and perhaps all dense cores with embedded infrared sources have outflows. L1681B contains an unresolved source with velocity extent and emission asymmetries which are consistent with gravitational infall.

Affiliated with

Also associated with

No associations

Rating

High-resolution CO observations of young low-mass stars 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 High-resolution CO observations of young low-mass stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High-resolution CO observations of young low-mass stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1874141