Molecular lines in 5 massive dense cores (Herpin, 2009)

Details Molecular lines in 5 massive dense cores (Herpin, 2009) Molecular lines in 5 massive dense cores (Herpin, 2009)

Jul 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ycat..35040853h&link_type=abstract

VizieR On-line Data Catalog: J/A+A/504/853. Originally published in: 2009A&A...504..853H

Physics

Interstellar Medium, Infrared Sources, Line Profiles

Scientific paper

The figure 14-17 show some line profiles (not shown in the paper) from observations with the IRAM-30m and CSO telescopes (all observational parameters can be found in the Table 2 of the paper). The reduced data for all the observed lines are given in the individual fit files, labelled as follows: os-l.fit, where "o" represents the observed source and is "i1" for IRAS05358+3543, "i2" for IRAS18162-2048, "i3" for IRAS18264-1152, and "w" for W43MM1, respectively; "s" is the species (e.g. CS); "l" is the first number (level) of the line transition (e.g. "3" for "3-2"). The Tables 6-9 give all the parameters for the observed line emissions. Table 10 shows the opacities derived from modeling the molecular emission of the sources.
(6 data files).

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