ASTE Submillimeter Observations of a Young Stellar Object Condensation in Cederblad 110

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

30pages, 7 figures, Accepted for publication in ApJ

Scientific paper

10.1086/519269

We present results of submillimeter observations of a low-mass young stellar objects (YSOs) condensation in the Cederblad 110 region of the Chamaeleon I dark cloud with Atacama Submillimeter Telescope Experiment. Our HCO+(J=4-3) map reveals a dense molecular gas with an extent of ~ 0.1 pc, which is a complex of two envelopes associated with class I sources Ced110 IRS4 and IRS11 and a very young object Cha-MMS1. The other two class I sources in this region, IRS6 and NIR89, are located outside the clump and have no extended HCO+ emission. HCO+ abundance is calculated to be 2.6 x 10^{-10} for MMS1 and 3.4 x 10^{-9} for IRS4, which are comparable to the reported value for other young sources. Bipolar outflows from IRS4 and IRS6 are detected in our 12CO(J=3-2) map. The outflow from IRS4 seems to collide with Cha-MMS1. The outflow has enough momentum to affect gas motion in MMS1, although no sign has been detected to indicate that a triggered star formation has occurred.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

ASTE Submillimeter Observations of a Young Stellar Object Condensation in Cederblad 110 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 ASTE Submillimeter Observations of a Young Stellar Object Condensation in Cederblad 110, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and ASTE Submillimeter Observations of a Young Stellar Object Condensation in Cederblad 110 will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-457071

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.