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Cold Dust and its Heating Sources in M 33

Published online by Cambridge University Press:  05 December 2011

Shinya Komugi ,
Tomoka Tosaki ,
Kotaro Kohno ,
Takashi Tsukagoshi ,
Yoichi Tamura ,
Rie Miura ,
Sachiko Onodera ,
Nario Kuno ,
Ryohei Kawabe  and
Koichiro Nakanishi
...Show all authors
Shinya Komugi
Affiliation:
Joint ALMA Observatory, Alonso de Cordova 3107, Vitacura, Santiago, Chile, email: [email protected] National Astronomical Observatory of Japan, Osawa 2-21-1, Mitaka, Tokyo, Japan
Tomoka Tosaki
Affiliation:
Joetsu Univ. of Education, Yamayashiki-machi, Joetsu, Niigata, 943-8512, Japan
Kotaro Kohno
Affiliation:
Institute of Astronomy, School of Science, The University of Tokyo, Osawa, Mitaka, Tokyo, 181-0015, Japan Research Center for Early Universe, School of Science, The University of Tokyo, Hongo, Bunkyo, Tokyo, 113-033, Japan
Takashi Tsukagoshi
Affiliation:
Institute of Astronomy, School of Science, The University of Tokyo, Osawa, Mitaka, Tokyo, 181-0015, Japan
Yoichi Tamura
Affiliation:
Institute of Astronomy, School of Science, The University of Tokyo, Osawa, Mitaka, Tokyo, 181-0015, Japan
Rie Miura
Affiliation:
University of Tokyo, Department of Astronomy, School of Science, Hongo, Bunkyo, Tokyo, 113-0033, Japan
Sachiko Onodera
Affiliation:
Nobeyama Radio Observatory, National Astronomical Observatory of Japan, Minamimaki, Minamisaku, Nagano, 384-1305, Japan
Nario Kuno
Affiliation:
Nobeyama Radio Observatory, National Astronomical Observatory of Japan, Minamimaki, Minamisaku, Nagano, 384-1305, Japan
Ryohei Kawabe
Affiliation:
Nobeyama Radio Observatory, National Astronomical Observatory of Japan, Minamimaki, Minamisaku, Nagano, 384-1305, Japan
Koichiro Nakanishi
Affiliation:
National Astronomical Observatory of Japan, Osawa 2-21-1, Mitaka, Tokyo, Japan
Tsuyoshi Sawada
Affiliation:
Joint ALMA Observatory, Alonso de Cordova 3107, Vitacura, Santiago, Chile, email: [email protected] National Astronomical Observatory of Japan, Osawa 2-21-1, Mitaka, Tokyo, Japan
Hajime Ezawa
Affiliation:
National Astronomical Observatory of Japan, Osawa 2-21-1, Mitaka, Tokyo, Japan
Grant W. Wilson
Affiliation:
Department of Astronomy, University of Massachusetts, Amherst, Massachusetts 01003, USA
Min S. Yun
Affiliation:
Department of Astronomy, University of Massachusetts, Amherst, Massachusetts 01003, USA
Kimberly S. Scott
Affiliation:
Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USA
David H. Hughes
Affiliation:
Instituto Nacional de Astrofisica, Optica y Electronica (INAOE), Aptdo. Postal 51 7216, 72000 Puebla, Mexico
Itziar Aretxaga
Affiliation:
Instituto Nacional de Astrofisica, Optica y Electronica (INAOE), Aptdo. Postal 51 7216, 72000 Puebla, Mexico
Thushara A. Perera
Affiliation:
Department of Physics, Illinois Wesleyan University, Bloomington, Illinois 6172-2900, USA
Jason E. Austermann
Affiliation:
Center for Astrophysics and Space Astronomy, University of Colorado, Boulder, Colorado 80309, USA
Kunihiko Tanaka
Affiliation:
Department of Physics, Keio University, 3-14-1 Yokohama, Kanagawa, Japan
Kazuyuki Muraoka
Affiliation:
Department of Physical Science, Osaka Prefecture University, 1-1 Sakai, Osaka, Japan
Fumi Egusa
Affiliation:
Institute of Space and Astronautical Science, Japan Space Exploration Agency, 3-1-1 Yoshinodai, Chuo-ku, Sagamihara, Kanagawa, Japan
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Abstract

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We have mapped the nearby face-on spiral galaxy M 33 in the 1.1 mm dust continuum using AzTEC on Atacama Submillimeter Telescope Experiment (ASTE). The preliminary results are presented here. The observed dust has a characteristic temperature of ~ 21 K in the central kpc, radially declining down to ~ 13 K at the edge of the star forming disk. We compare the dust temperatures with KS band flux and star formation tracers. Our results imply that cold dust heating may be driven by long-lived stars even nearby star forming regions.

Keywords

(ISM:) dustgalaxies: ISM
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S277: Tracing the Ancestry of Galaxies (on the land of our ancestors) , December 2010 , pp. 26 - 29
Copyright
Copyright © International Astronomical Union 2011

References

Bianchi, S., Davies, J. I., & Alton, P. B. 2000, A&A, 359, 65Google Scholar
Calzetti, D., et al. 2007, ApJ, 666, 870CrossRefGoogle Scholar
Devereux, N., Duric, N., & Scowen, P. A. 1997, AJ, 113, 236CrossRefGoogle Scholar
Draine, B. T. & Lee, H. M. 1984, ApJ, 285, 89CrossRefGoogle Scholar
Ezawa, H., Kawabe, R., Kohno, K., & Yamamoto, S. 2004, Proc. SPIE, 5489, 763CrossRefGoogle Scholar
Ezawa, H., et al. 2008, Proc. SPIE, 7012Google Scholar
Kohno, K. 2005, ASP Conf. Ser. 344, 242Google Scholar
Onodera, S., et al. 2010, ApJ, 722, L127CrossRefGoogle Scholar
Tosaki, T., et al. 2011, PASJ, submittedGoogle Scholar
Walterbos, R. A. M. & Greenawalt, B. 1996, ApJ, 460, 696CrossRefGoogle Scholar
Wilson, G. W., et al. 2008, MNRAS, 386, 807CrossRefGoogle Scholar
Xu, C. & Helou, G. 1996, ApJ, 456, 163CrossRefGoogle Scholar