Multiple HC3N line observations towards 19 Galactic massive star-forming regions

نویسندگان

چکیده

We performed observations of the HC$_3$N (24-23, 17-16, 11-10, 8-7) lines towards a sample consisting 19 Galactic massive star-forming regions with Arizona Radio Observatory 12-m and Caltech Submillimeter 10.4-m telescopes. were detected in sources except for W44, where only (17-16, 11-10) detected. Twelve nineteen showed probable line wing features. The excitation temperatures estimated from ratio (24-23) to (17-16) 18 are range 23-57 K. widths higher-$J$ transitions larger than lower-$J$ ones most sources. This indicates that inner dense warm have more violent turbulence or other motions (such as rotation) outer these A possible cutoff tendency was found around $L_{\rm IR}$ $\sim$ 10$^{6}$ $L_\odot$ relation between full width at half maximum widths.

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ژورنال

عنوان ژورنال: Publications of the Astronomical Society of Japan

سال: 2021

ISSN: ['2053-051X', '0004-6264']

DOI: https://doi.org/10.1093/pasj/psab012