(C-13)O and HCO(+) observations of IRAS sources in L1641

Details (C-13)O and HCO(+) observations of IRAS sources in L1641 (C-13)O and HCO(+) observations of IRAS sources in L1641

Oct 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...398..544c&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 398, no. 2, p. 544-551.

Astronomy and Astrophysics

Astronomy

25

Carbon Monoxide, Formaldehyde, Infrared Sources (Astronomy), Molecular Ions, Radio Astronomy, Infrared Astronomy Satellite, Molecular Flow, Molecular Gases, Orion Nebula, Spatial Distribution, Star Formation

Scientific paper

Twenty-eight IRAS sources selected from the IRAS co-added images in L1641 were observed in the (C-13)O (J = 1-0) and HCO(+) (J = 1-0) using the 45 m telescope at the Nobeyama Radio Observatory. The (C-13)O and HCO(+) column densities toward the IRAS sources correlated with each other, and both column densities also correlated with the IRAS color defined by the 12-25-micron flux ratio. Three outflow sources mapped in this study showed well-defined HCO(+) cores with a size of 0.1 pc and a mass of 3-30 solar masses. The most probable explanation of these results is that the molecular dense cores are dissipated by both accretion and outflow during an early stage of stellar evolution.

Affiliated with

Also associated with

No associations

Rating

(C-13)O and HCO(+) observations of IRAS sources in L1641 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 (C-13)O and HCO(+) observations of IRAS sources in L1641, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and (C-13)O and HCO(+) observations of IRAS sources in L1641 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1869646