H13CN–HN13C Intensity Ratio as a Temperature Indicator of Interstellar Clouds

نویسندگان

چکیده

With the 30-m IRAM radio telescope, we observed several massive star forming regions at wavelengths of 3–4 and 2 mm. The temperature gas in sources was estimated from lines CH3CCH transitions NH3 molecule obtained during observations 100-m telescope Effelsberg. As a result, correlation between integrated intensity ratios J = 1−0 H13CN–HN13C kinetic has been obtained. results allow us to propose use ratio as possible indicator interstellar clouds. We also compared estimates with dust $${{T}_{{{\text{dust}}}}}$$ . no significant found.

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ژورنال

عنوان ژورنال: Astronomy Reports

سال: 2022

ISSN: ['1562-6881', '1063-7729']

DOI: https://doi.org/10.1134/s1063772922110154