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Maser Tracers of Gas Dynamics near Young Stars New Perspectives

Published online by Cambridge University Press:  07 February 2024

Alberto Sanna Open the ORCID record for Alberto Sanna [Opens in a new window]  and
Luca Moscadelli Open the ORCID record for Luca Moscadelli [Opens in a new window]
Alberto Sanna*
Affiliation:
INAF, Osservatorio Astronomico di Cagliari, via della Scienza 5, 09047, Selargius, Italy.
Luca Moscadelli
Affiliation:
INAF, Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Firenze, Italy
*
email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

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The protostellar environment where young stars form has physical conditions suitable to excite a number of molecular maser lines that have traditionally provided an unique probe of star formation kinematics, at the highest angular resolution of radio very long baseline interferometry (VLBI) observations. In the following, we will discuss a number of recent results on our understanding of the gas dynamics traced by masers in the vicinity of young forming stars. These findings provide direct clues on how our community can substantially contribute to the field of star formation in the next decade.

Keywords

MasersStars: formationISM: kinematics and dynamics
Type
Contributed Paper
Information
Proceedings of the International Astronomical Union , Volume 18 , Symposium S380: Cosmic Masers: Proper Motion toward the Next-Generation Large Projects , December 2022 , pp. 159 - 166
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Creative Commons
Creative Common License - CCCreative Common License - BY
This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted re-use, distribution and reproduction, provided the original article is properly cited.
Copyright
© The Author(s), 2024. Published by Cambridge University Press on behalf of International Astronomical Union

References

Bartkiewicz, A., Sanna, A., Szymczak, M., et al. 2020, A&A, 637, A15 Google Scholar
Cragg, D. M., Johns, K. P., Godfrey, P. D., et al. 1992, MNRAS, 259, 203 10.1093/mnras/259.1.203CrossRefGoogle Scholar
Cragg, D. M., Sobolev, A. M., & Godfrey, P. D. 2005, MNRAS, 360, 533 10.1111/j.1365-2966.2005.09077.xCrossRefGoogle Scholar
Elitzur, M., Hollenbach, D. J., & McKee, C. F. 1989, ApJ, 346, 983 10.1086/168080CrossRefGoogle Scholar
Elitzur, M., Hollenbach, D. J., & McKee, C. F. 1992, ApJ, 394, 221 10.1086/171574CrossRefGoogle Scholar
Genzel, R., Reid, M. J., Moran, J. M., et al. 1981, ApJ, 244, 884 10.1086/158764CrossRefGoogle Scholar
Goddi, C., Moscadelli, L., & Sanna, A. 2011, A&A, 535, L8 Google Scholar
Gwinn, C. R., Moran, J. M., & Reid, M. J. 1992, ApJ, 393, 149 10.1086/171493CrossRefGoogle Scholar
Hollenbach, D., Elitzur, M., & McKee, C. F. 2013, ApJ, 773, 70 10.1088/0004-637X/773/1/70CrossRefGoogle Scholar
Kaufman, M. J. & Neufeld, D. A. 1996, ApJ, 456, 250 10.1086/176645CrossRefGoogle Scholar
Menten, K. M. 1991, ApJL, 380, L75 10.1086/186177CrossRefGoogle Scholar
Minier, V., Booth, R. S., & Conway, J. E. 2002, A&A, 383, 614 Google Scholar
Moscadelli, L., Cesaroni, R., Rioja, M. J., et al. 2011, A&A, 526, A66 Google Scholar
Moscadelli, L., Sanna, A., & Goddi, C. 2011, A&A, 536, A38 Google Scholar
Moscadelli, L., Li, J. J., Cesaroni, R., et al. 2013, A&A, 549, A122 Google Scholar
Moscadelli, L., Sánchez-Monge, Á., Goddi, C., et al. 2016, A&A, 585, A71 Google Scholar
Moscadelli, L., Sanna, A., Goddi, C., et al. 2019, A&A, 631, A74 Google Scholar
Moscadelli, L., Sanna, A., Goddi, C., et al. 2020, A&A, 635, A118 Google Scholar
Moscadelli, L., Sanna, A., Beuther, H., et al. 2022, Nature Astronomy, 6, 1068 10.1038/s41550-022-01754-4CrossRefGoogle Scholar
Reid, M. J., Menten, K. M., Brunthaler, A., et al. 2014, ApJ, 783, 130 10.1088/0004-637X/783/2/130CrossRefGoogle Scholar
Sanna, A., Moscadelli, L., Cesaroni, R., et al. 2010, A&A, 517, A71 Google Scholar
Sanna, A., Moscadelli, L., Cesaroni, R., et al. 2010, A&A, 517, A78 Google Scholar
Sanna, A., Moscadelli, L., Surcis, G., et al. 2017, A&A, 603, A94 Google Scholar
Sanna, A., Moscadelli, L., Goddi, C., et al. 2018, A&A, 619, A107 Google Scholar
Sanna, A., Moscadelli, L., Goddi, C., et al. 2019, A&A, 623, L3 Google Scholar
Sanna, A., Giannetti, A., Bonfand, M., et al. 2021, A&A, 655, A72 Google Scholar
Sobolev, A. M., Cragg, D. M., & Godfrey, P. D. 1997, A&A, 324, 211 Google Scholar
Sugiyama, K., Fujisawa, K., Doi, A., et al. 2014, A&A, 562, A82 Google Scholar
Zinchenko, I., Liu, S.-Y., Su, Y.-N., et al. 2018, IAU Symposium, 332, 270 Google Scholar