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Star formation feedback onto molecular clouds of KAGONMA sources using temperature distribution

Published online by Cambridge University Press:  09 June 2023

N. Takeba Open the ORCID record for N. Takeba [Opens in a new window] ,
T. Handa Open the ORCID record for T. Handa [Opens in a new window] ,
T. Murase Open the ORCID record for T. Murase [Opens in a new window] ,
M. Kohno ,
T. Omodaka ,
M. Nakano ,
Y. Hirata ,
J. O. Chibueze Open the ORCID record for J. O. Chibueze [Opens in a new window]  and
R. A. Burns
N. Takeba
Affiliation:
Faculty of Science, Kagoshima University, 1-21-35 Korimoto, Kagoshima 890-0065, Japan. email: n34.bamu.lss@gmail.com
T. Handa
Affiliation:
Faculty of Science, Kagoshima University, 1-21-35 Korimoto, Kagoshima 890-0065, Japan. email: n34.bamu.lss@gmail.com
T. Murase
Affiliation:
Faculty of Science, Kagoshima University, 1-21-35 Korimoto, Kagoshima 890-0065, Japan. email: n34.bamu.lss@gmail.com
M. Kohno
Affiliation:
Astronomy Section, Nagoya City Science Museum, 2-17-1 Sakae, Naka-ku, Nagoya, Aichi 460-0008, Japan. Department of Physics, Graduate School of Science, Nagoya University, Furo-cho, Chikusa-ku, Nagoya, Aichi 464-8602, Japan.
T. Omodaka
Affiliation:
Faculty of Science, Kagoshima University, 1-21-35 Korimoto, Kagoshima 890-0065, Japan. email: n34.bamu.lss@gmail.com
M. Nakano
Affiliation:
Faculty of Education, Oita University, 700 Dannoharu, Oita 870-1192, Japan.
Y. Hirata
Affiliation:
Faculty of Science, Kagoshima University, 1-21-35 Korimoto, Kagoshima 890-0065, Japan. email: n34.bamu.lss@gmail.com
J. O. Chibueze
Affiliation:
Centre for Space Research, Potchefstroom campus, North-West University, Potchefstroom 2531, South Africa Department of Phys. and Astron., Faculty of Physical Sci., Univ. of Nigeria, Carver Building, University road, Nsukka 410001, Nigeria
R. A. Burns
Affiliation:
National Astronomical Observatory of Japan (NAOJ), 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan
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Abstract

This paper reports on four of the sources observed in the KAGONMA (KAgoshima Galactic Object survey with the Nobeyama 45-m telescope by Mapping in Ammonia lines) project for which mapping observations have been completed (KAG35, KAG45, KAG64, and KAG71). In this study, we compiled the analysis results of four sources for which mapping observations were completed in the KAGONMA project and statistically investigated the range to which star formation activity affects the molecular gas. In order to investigate the affected range, we analyzed the heating range by focusing on the temperature distribution of the molecular cloud and found that it is within about 3 pc. This suggests that direct star formation feedback in molecular clouds is very spatially limited.

Keywords

ISM: clouds – Hii regions
Type
Poster Paper
Information
Proceedings of the International Astronomical Union , Volume 17 , Symposium S373: Resolving the Rise and Fall of Star Formation in Galaxies , August 2021 , pp. 154 - 156
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Copyright
© The Author(s), 2023. Published by Cambridge University Press on behalf of International Astronomical Union

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References

Planck Collaboration 2011, A&A, 536, A25 Google Scholar