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Early Star Formation Traced by Water Masers

Published online by Cambridge University Press:  07 February 2024

Dmitry Ladeyschikov Open the ORCID record for Dmitry Ladeyschikov [Opens in a new window]
Dmitry Ladeyschikov*
Affiliation:
Astronomical Observatory, Institute for Natural Sciences and Mathematics, Ural Federal University, 19 Mira street, Ekaterinburg, 620002, Russia.
*
email: dmitry.ladeyschikov@urfu.ru
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Abstract

In this study, the correlation between 22 GHz water masers and other maser species with far infrared/submillimeter (FIR/sub-mm) sources is investigated. Comparing luminosity to mass ratio (L/M) of FIR/sub-mm clumps linked to different maser species, 22 GHz water masers have significantly lower L/M values than 6.7 GHz methanol and 1665 MHz OH masers. This suggests 22 GHz water masers may precede them in the evolution timeline of SFRs. The close association between water masers and FIR/sub-mm sources provides insight into maser pumping conditions and evolutionary stages.

Keywords

Masersstar formation regionHi-GALATLASGALevolution timeline
Type
Poster 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. 230 - 231
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Copyright
© The Author(s), 2024. Published by Cambridge University Press on behalf of International Astronomical Union

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References

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