Physics
Scientific paper
Jul 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000ycat..33611079z&link_type=abstract
VizieR On-line Data Catalog: J/A+A/361/1079. Originally published in: 2000A&A...361.1079Z
Physics
Molecular Clouds, Radio Lines
Scientific paper
We surveyed 81 dense molecular cores associated with regions of massive star formation and Sgr A in the J(K-1K1)=5(05)-4(04) and 10(010)-9(09)_ lines of HNCO. Line emission was detected towards 57 objects. Selected subsamples were also observed in the 1(01)-0(00), 4(04)-3(03), 7(07)-6(06), 15(015)-14(014), 16(016)-15(015) and 21(021)-20(020) lines, covering a frequency range from 22 to 461 GHz. HNCO lines from the K_(-1)=2,3 ladders were detected in several sources. Towards Orion-KL, K_(-1)=5 transitions with upper state energies E_u/k~1100 and 1300K could be observed. The tables contain the source lists and the results of these SEST observations. (15 data files).
Henkel Carsten
Mao Rui-Qing
Zinchenko I. I.
No associations
LandOfFree
HNCO in massive galactic dense cores (Zinchenko, 2000) 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 HNCO in massive galactic dense cores (Zinchenko, 2000), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and HNCO in massive galactic dense cores (Zinchenko, 2000) will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1484372