The evolutionary status of young stellar mass loss driving sources as derived from IRAS observations

Details The evolutionary status of young stellar mass loss driving sources as derived from IRAS observations The evolutionary status of young stellar mass loss driving sources as derived from IRAS observations

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mnras.237....1b&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 237, March 1, 1989, p. 1-15.

Astronomy and Astrophysics

Astronomy

38

Early Stars, Herbig-Haro Objects, Infrared Astronomy Satellite, Stellar Evolution, Stellar Mass Ejection, Accretion Disks, Far Infrared Radiation, Molecular Flow, Star Formation

Scientific paper

A statistical analysis of the IRAS data for young stellar objects associated with mass outflows (Herbig-Haro objects and molecular outflows) is presented. Systematic differences are found between the observed far-infrared behavior and that predicted by a model describing the main accretion phase during the formation of low-mass stars. It is suggested that the low-mass outflow sources are at a later evolutionary stage and not truly protostellar.

Affiliated with

Also associated with

No associations

Rating

The evolutionary status of young stellar mass loss driving sources as derived from IRAS observations 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 The evolutionary status of young stellar mass loss driving sources as derived from IRAS observations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The evolutionary status of young stellar mass loss driving sources as derived from IRAS observations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1807081