[OI] (63microns) Determined Mass-Loss Rates in Young Stellar Objects

Details [OI] (63microns) Determined Mass-Loss Rates in Young Stellar Objects [OI] (63microns) Determined Mass-Loss Rates in Young Stellar Objects

Dec 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aas...183.8103r&link_type=abstract

American Astronomical Society, 183rd AAS Meeting, #81.03; Bulletin of the American Astronomical Society, Vol. 25, p.1419

Astronomy and Astrophysics

Astronomy

Scientific paper

We present a method for determining the instantaneous mass-loss rate from a forming star using observations of the fine-structure [OI] (63microns) line (Hollenbach 1985), and compare it to the CO method for determining mass-loss rates. In addition we present observations of three young outflows, VLA 1623 and IRAS 16293-2422, located in the rho Oph star-forming cloud, and L1448, located in the NGC 1333 star-forming cloud, and determine mass-loss rates for these three outflows.

Affiliated with

Also associated with

No associations

Rating

[OI] (63microns) Determined Mass-Loss Rates in Young Stellar Objects 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 [OI] (63microns) Determined Mass-Loss Rates in Young Stellar Objects, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and [OI] (63microns) Determined Mass-Loss Rates in Young Stellar Objects will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-780489