An interferometric study of the low-mass protostar IRAS 16293-2422: small scale organic chemistry

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

11 pages, 15 figures, accepeted by A&A

Scientific paper

10.1051/0004-6361:200809673

Aims: To investigate the chemical relations between complex organics based on their spatial distributions and excitation conditions in the low-mass young stellar objects IRAS 16293-2422 A and B. Methods: Interferometric observations with the Submillimeter Array have been performed at 5''x3'' resolution revealing emission lines of HNCO, CH3CN, CH2CO, CH3CHO and C2H5OH. Rotational temperatures are determined from rotational diagrams when a sufficient number of lines are detected. Results: Compact emission is detected for all species studied here. For HNCO and CH3CN it mostly arises from source A, CH2CO and C2H5OH have comparable strength for both sources and CH3CHO arises exclusively from source B. HNCO, CH3CN and CH3CHO have rotational temperatures >200 K. The (u,v)-visibility data reveal that HNCO also has extended cold emission. Conclusions: The abundances of the molecules studied here are very similar within factors of a few to those found in high-mass YSOs. Thus the chemistry between high- and low-mass objects appears to be independent of luminosity and cloud mass. Bigger abundance differences are seen between the A and B source. The HNCO abundance relative to CH3OH is ~4 times higher toward A, which may be due to a higher initial OCN- ice abundances in source A compared to B. Furthermore, not all oxygen-bearing species are co-existent. The different spatial behavior of CH2CO and C2H5OH compared with CH3CHO suggests that hydrogenation reactions on grain-surfaces are not sufficient to explain the observed gas phase abundances. Selective destruction of CH3CHO may result in the anti-coincidence of these species in source A. These results illustrate the power of interferometric compared with single dish data in terms of testing chemical models.

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

An interferometric study of the low-mass protostar IRAS 16293-2422: small scale organic chemistry 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 An interferometric study of the low-mass protostar IRAS 16293-2422: small scale organic chemistry, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and An interferometric study of the low-mass protostar IRAS 16293-2422: small scale organic chemistry will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-688101

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