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A sensitive survey for water masers towards Bok globules

Published online by Cambridge University Press:  01 March 2007

I. de Gregorio-Monsalvo ,
J. F. Gómez ,
O. Suárez ,
T. B. H. Kuiper ,
G. Anglada ,
N. A. Patel  and
J. M. Torrelles
I. de Gregorio-Monsalvo
Affiliation:
European Southern Observatory, Alonso de Córdova 3107, Vitacura, Santiago, Chile, email: [email protected].
J. F. Gómez
Affiliation:
Instituto de Astrofísica de Andalucìa (CSIC), Apartado 3004, E-18080 Granada, Spain.
O. Suárez
Affiliation:
Laboratorio de Astrofísica Espacial y Fìsica Fundamental (INTA), Apartado 50727, E-28080 Madrid, Spain.
T. B. H. Kuiper
Affiliation:
Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA.
G. Anglada
Affiliation:
Instituto de Astrofísica de Andalucìa (CSIC), Apartado 3004, E-18080 Granada, Spain.
N. A. Patel
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA.
J. M. Torrelles
Affiliation:
Instituto de Ciencias del Espacio (CSIC) and Institut d'Estudis Espacials de Catalunya, Facultat de Fìsica, Planta 7, Universitat de Barcelona, Av. Diagonal 647, E-08028 Barcelona, Spain
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Abstract

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In this work we report the most sensitive water maser survey towards Bok globules to date, using NASA's 70 m antenna in Robledo de Chavela (Spain). We observed 207 positions within the Clemens & Barvainis catalog that show indications of possible star formation or with a high probability of harboring a young stellar object. With this survey we have increased the number of Bok globules known to present water maser emission from three to nine. We have complemented these results with interferometric high-angular resolution observations towards some of our detections.

Keywords

ISM: globulesISM:moleculesmasersstars:formationsurveys
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 3 , Symposium S242: Astrophysical Masers and their Environments , March 2007 , pp. 146 - 147
Copyright
Copyright © International Astronomical Union 2008

References

Bok, B. J., & Reilly, E. F. 1947, ApJ 105, 255CrossRefGoogle Scholar
Claussen, M. J., Marvel, K. B., Wootten, A., & Wilking, B. A. 1998, ApJ, 507, L79CrossRefGoogle Scholar
Clemens, D. P. & Barvainis, R. 1988, ApJS, 68, 257CrossRefGoogle Scholar
de Gregorio-Monsalvo, I., Gómez, J. F., Suárez, O., Kuiper, T. B. H., Anglada, G., Patel, N. A., & Torrelles, J. M. 2006, AJ 132, 2584CrossRefGoogle Scholar
Gómez, J. F., de Gregorio-Monsalvo, I., Suárez, O, & Kuiper, T. B. H. 2006, AJ 132, 1322CrossRefGoogle Scholar
Moscadelli, L., Testi, L., Furuya, R. S., Goddi, C., Claussen, M., Kitamura, Y., & Wootten, A. 2006, A&A 446, 985Google Scholar
Yun, J. L., & Clemens, D. P. 1992, ApJ, 385, L21CrossRefGoogle Scholar