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Extragalactic class I methanol maser: A new probe for starbursts and feedback of galaxies

Published online by Cambridge University Press:  16 July 2018

Xi Chen  and
Simon P. Ellingsen
Xi Chen
Affiliation:
Center for Astrophysics, GuangZhou University, Guangzhou, 510006, China email: [email protected] Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, China email: [email protected]
Simon P. Ellingsen
Affiliation:
School of Physical Sciences, University of Tasmania, Hobart, Tasmania, Australia email: [email protected]
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Abstract

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We report progress on research relating to 36.2 GHz extragalactic class I methanol masers, including a review of published work and new observations at high angular resolution. These observations reveal that extragalactic class I masers are excited in shocked gas and maybe associated with starbursts, galactic-scale outflows from active galactic nuclei (AGNs) feedback, or the inner-end region of the galactic bar. The current observational results suggests that extragalactic class I methanol masers provide a new probe for starbursts and feedback in active galaxies.

Keywords

masersstars: formationISM: moleculesgalaxies
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 13 , Symposium S336: Astrophysical Masers: Unlocking the Mysteries of the Universe , September 2017 , pp. 99 - 104
Copyright
Copyright © International Astronomical Union 2018 

References

Batrla, W. & Menten, K. M., 1988, Ap. Lett., 329, 117Google Scholar
Caswell, J. L., Fuller, G. A., Green, J. A., et al., 2010, MNRAS, 404, 1029Google Scholar
Chen, X., Ellingsen, S. P., Baan, W. A., et al., 2015, Ap. Lett., 800, 2Google Scholar
Chen, X., Ellingsen, S. P., Gan, C. G., et al., 2014, ChSBu, 59, 1066Google Scholar
Chen, X., Ellingsen, S. P., Zhang, J. S., et al., 2016, MNRAS, 459, 357Google Scholar
Cicone, C., Feruglio, C., Maiolino, R., et al., 2012, A&A, 543, A99Google Scholar
Darling, J., Goldsmith, P., Li, D., & Giovanelli, R., 2003, AJ, 125, 1177Google Scholar
Green, J. A., Caswell, J. L., Fuller, G. A., et al., 2009, MNRAS, 392, 783CrossRefGoogle Scholar
Green, J. A., Caswell, J. L., Fuller, G. A., et al., 2008, MNRAS, 385, 948Google Scholar
Ellingsen, S. P., 2006, ApJ, 638, 241CrossRefGoogle Scholar
Ellingsen, S. P., Breen, S. L., Caswell, J. L., Quinn, L. J., & Fuller, G. A., 2010, MNRAS, 404, 779Google Scholar
Ellingsen, S. P., Chen, X., Breen, S. L., & Qiao, H.-H., 2017, MNRAS, 472, 604Google Scholar
Ellingsen, S. P., Chen, X., Qiao, H. Q., et al., 2014, Ap. Lett., 790, 28Google Scholar
Ellingsen, S. P., Norris, R. P., Whiteoak, J. B., et al., 1994, MNRAS, 267, 510Google Scholar
Ellingsen, S. P., Sobolev, A. M., Cragg, D. M., et al., 2012, Ap. Lett., 759, 5Google Scholar
McCarthy, T. P., Ellingsen, S. P., Chen, X. et al., 2017, Ap. Lett., 846, 156Google Scholar
McDowell, J. C., Clements, D. L., Lamb, S. A., et al., 2003, ApJ, 591, 154Google Scholar
Menten, K. M., 1991, Ap. Lett., 380, 75CrossRefGoogle Scholar
Phillips, C. J., Norris, R. P., Ellingsen, S. P., & Rayner, D. P., 1998, MNRAS, 294, 265Google Scholar
Sjouwerman, L. O., Murray, C. E., Pihlströ, Y. M., Fish, V. L., & Araya, E. D., 2010, Ap. Lett., 724, 158Google Scholar
Sobolev, A. M., 1993, Astron. Lett., 19, 293Google Scholar
Voronkov, M. A., Brooks, K. J., Sobolev, A. M., et al., 2006, MNRAS, 373, 411CrossRefGoogle Scholar
Yang, W. J., Xu, Y., Chen, X., et al., 2017, ApJS, 231, 20Google Scholar
Yusef-Zadeh, F., Cotton, W., Viti, S., Wardle, M., & Royster, M., 2013, Ap. Lett., 764, L19Google Scholar