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High-Temperature Chemistry in External Galaxies

Published online by Cambridge University Press:  04 September 2018

Nanase Harada
Nanase Harada*
Affiliation:
Academia Sinica Institute of Astronomy and Astrophysics Taipei, Taiwan email: harada@asiaa.sinica.edu.tw
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Abstract

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In external galaxies, some galaxies have higher activities of star formation and central supermassive black holes. The interstellar medium in those galaxies can be heated by different mechanisms such as UV-heating, X-ray heating, cosmic-ray heating, and shock/mechanical heating. Chemical compositions can also be affected by those heating mechanisms. Observations of many molecular species in those nearby galaxies are now possible with the high sensitivity of Atacama Large Millimeter/sub-millimeter Array (ALMA). Here I cover different chemical models for those heating mechanisms. In addition, I present recent ALMA results of extragalactic astrochemistry including our results of a face-on galaxy M83 and an infrared-luminous merger NGC 3256.

Keywords

galaxies: ISM galaxies: active ISM: molecules ISM: abundances astrochemistry
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 13 , Symposium S332: Astrochemistry VII: Through the Cosmos from Galaxies to Planets , March 2017 , pp. 25 - 36
Copyright
Copyright © International Astronomical Union 2018 

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