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44 GHz Methanol Maser Surveys

Published online by Cambridge University Press:  24 July 2012

S. E. Kurtz
S. E. Kurtz*
Affiliation:
Centro de Radioastronomía y Astrofísica, Universidad Nacional Autonoma de México (Morelia, Michoacán, México) email: [email protected]
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Abstract

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Class I 44 GHz methanol masers are not as well-known, as common, or as bright as their more famous Class II cousins at 6.7 and 12.2 GHz. Nevertheless, the 44 GHz masers are commonly found in high-mass star forming regions. At times they appear to trace dynamically important phenomena; at other times they show no obvious link to the star formation process. Here, we summarize the major observational efforts to date, including both dedicated surveys and collateral observations. The principal results are presented, some that were expected, and others that were unexpected.

Keywords

maserssurveysstars:formation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S287: Cosmic Masers - from OH to H0 , January 2012 , pp. 133 - 140
Copyright
Copyright © International Astronomical Union 2012

References

Araya, E., Hofner, P., Kurtz, S., Olmi, L., & Linz, H. 2008, ApJ 675, 420CrossRefGoogle Scholar
Araya, E., Kurtz, S., Hofner, P., & Linz, H. 2009, ApJ 698, 1321CrossRefGoogle Scholar
Bachiller, R., Gómez-González, J, Barcia, A., & Menten, K. M. 1990, A&A 240, 116Google Scholar
Bae, J.-H., Kim, K.-T., Youn, S.-Y., Kim, W.-J., Byun, D.-Y., Kang, H., & Oh, C. S. 2011, ApJS 196, 21CrossRefGoogle Scholar
Cesaroni, R., Felli, M., Testi, L., Walmsley, C. M., & Olmi, L. 1997, A&A, 325, 725Google Scholar
Cesaroni, R., Felli, M., Jenness, T., Neri, R., Olmi, L., Robberto, M., Testi, L., & Walmsley, C. M. 1999, A&A 345, 949Google Scholar
Cyganowski, C. J., Brogan, C. L., Hunter, T. R., & Churchwell, E. 2009, ApJ 702, 1615CrossRefGoogle Scholar
Cyganowski, C. J., Brogan, C. L., Hunter, T. R., & Churchwell, E. 2011, ApJ 743, 56CrossRefGoogle Scholar
Fontani, F., Cesaroni, R., & Furuya, R. S. 2010, A&A 517, 56Google Scholar
Haschick, A. D., Menten, K. M., & Baan, W. A. 1990, ApJ 354, 556CrossRefGoogle Scholar
Hoare, M. G., Kurtz, S. E., Lizano, S., Keto, E., & Hofner, P. 2007, in: Reipurth, B., Jewitt, D., & Keil, K. (eds.), Protostars and Planets V, (Tucson: University of Arizona Press), p. 181Google Scholar
Kalenskii, S. V., Bachiller, R., Berulis, I. I., Val'tts, I. E., Gómez-González, J., Martin-Pintado, J., Rodríguez-Franco, A., & Slysh, V. I. 1992, SvA 36, 517Google Scholar
Kalenskii, S. V., Promyslov, V. G., Slysh, V. I., Bergman, P., & Winnberg, A. 2006, Astron. Rep., 50, 289CrossRefGoogle Scholar
Kalenskii, S. V., Johansson, L. E. B., Bergman, P., Kurtz, S., Hofner, P., Walmsley, C. M., & Slysh, V. I. 2010a, MNRAS, 405, 613Google Scholar
Kalenskii, S. V., Kurtz, S., Slysh, V. I., Hofner, P., Walmsley, C. M., Johansson, L. E. B., & Bergman, P. 2010b, Astron. Rep., 54, 932CrossRefGoogle Scholar
Kogan, L. & Slysh, V. 1998, ApJ 497, 800CrossRefGoogle Scholar
Kurtz, S., Hofner, P., & Vargas-Álvarez, C. 2004, ApJS 155, 149CrossRefGoogle Scholar
Molinari, S., Brand, J., Cesaroni, R., & Palla, F. 1996 A&A 308, 573Google Scholar
Morimoto, M., Kanzawa, T., & Ohishi, M. 1985 ApJ (Letters) 288, L11CrossRefGoogle Scholar
Plambeck, R. L. & Menten, K. M. 1990, ApJ, 364, 555CrossRefGoogle Scholar
Pratap, P., Shute, P. A., Keane, T. C., & Battersby, C., Sterling, S. 2008, AJ 135, 1718CrossRefGoogle Scholar
Sridharan, T. K., Beuther, H., & Schilke, P. 2002, ApJ 566, 931CrossRefGoogle Scholar
Slysh, V. I., Kalenskii, S. V., Val'tts, I. E., & Otrupcek, R. 1994, Mon. Not. Royal Astron. Soc. 268, 464CrossRefGoogle Scholar
Val'tts, I. E. & Larionov, G. M. 2007 Astron. Rep. 51, 519CrossRefGoogle Scholar
Zhang, Q., Hunter, T. R., Brand, J., Sridharan, T. K., Cesaroni, R., Molinari, S., Wang, J., & Kramer, M. 2005, ApJ 625, 864CrossRefGoogle Scholar