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Search for molecular gas in XUV disk of M83

Published online by Cambridge University Press:  21 March 2017

Kana Morokuma-Matsui
Affiliation:
National Astronomical Observatory of Japan (NAOJ) email: kana.matsui@nao.ac.jp
Jin Koda
Affiliation:
Stony Brook University
Tatsuya Takekoshi
Affiliation:
National Astronomical Observatory of Japan (NAOJ) email: kana.matsui@nao.ac.jp
Masao Saito
Affiliation:
National Astronomical Observatory of Japan (NAOJ) email: kana.matsui@nao.ac.jp
Hiroyuki Nakanishi
Affiliation:
Kagoshima University
Samuel Boissier
Affiliation:
Laboratoire d’Astrophysique de Marseille
Barry F. Madore
Affiliation:
Carnegie Observatories
Alessandro Boselli
Affiliation:
Laboratoire d’Astrophysique de Marseille
Armando Gil de Paz
Affiliation:
Universidad Complutense de Madrid
David Thilker
Affiliation:
Johns Hopkins University
Masafumi Yagi
Affiliation:
National Astronomical Observatory of Japan (NAOJ) email: kana.matsui@nao.ac.jp
Kazuo Sorai
Affiliation:
Hokkaido University
Nario Kuno
Affiliation:
University of Tsukuba
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Abstract

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We report a non-detection of CO(J=1-0) emission from one of the brightest Hii regions in the extended UV (XUV) disks of M 83 with on-source integration time of 11 hours.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2017 

References

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Koda, J. et al. 2012, ApJ, 749, 20 Google Scholar