Search for molecular outflows toward the pre-main-sequence objects
Creators
- 1. Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (USA)
- 2. Texas Univ., Austin (USA)
Description
A search for molecular outflows has been conducted toward a sample of 71 young stellar objects dominated by optically selected pre-main-sequence stars. Molecular outflows ranging in size from 0.07 to about 5 pc, with expansion velocities from 6 to 60 km/s, have been detected toward 20 of these objects and in an additional six infrared objects not included in the original survey. The apparent ages of the outflows are from 1000 to 500,000 yr; about half of the observed outflows are bipolar, with the rest showing a wide variety of morphologies. It is found that outflows driven by low-luminosity objects tend to be more bipolar than those driven by high-luminosity objects. The implications of the results of the study are discussed. 115 references
Additional details
Publishing Information
- Journal Title
- Astrophysical Journal, Supplement Series
- Journal Volume
- 67
- Series
- Astrophys. J., Suppl. Ser.
- Journal Page Range
- 283-371
- ISSN
- 0067-0049
- CODEN
- APJSA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 20000938
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- AGE ESTIMATION; CARBON MONOXIDE; COSMIC GASES; GAS FLOW; INFRARED RADIATION; INTERSTELLAR SPACE; MASS TRANSFER; MOLECULES; MORPHOLOGICAL CHANGES; PROTOSTARS
- Descriptors DEC
- CARBON COMPOUNDS; CARBON OXIDES; CHALCOGENIDES; ELECTROMAGNETIC RADIATION; FLUID FLOW; FLUIDS; GASES; OXIDES; OXYGEN COMPOUNDS; RADIATIONS; SPACE