Published in

Cambridge University Press, Proceedings of the International Astronomical Union, S370(17), p. 91-93, 2021

DOI: 10.1017/s1743921322004355

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Water and silicon-monoxide masers monitored towards the “water fountain” sources

Journal article published in 2021 by H. Imai ORCID, K. Amada ORCID, J. F. Gómez, L. Uscanga ORCID, D. Tafoya, K. Nakashima, K.-Y. Shum ORCID, Y. Hamae, R. Burns, G. Orosz ORCID
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Abstract

AbstractWe have investigated the evolution of 12 “water fountain” sources in real time in the accompanying H2O 2o and SiO masers through our FLASHING (Finest Legacy Acquisitions of SiO-/ H2O 2o-maser Ignitions by Nobeyama Generation) project. It has been confirmed that these masers are excellent probes of new jet blob ejections, acceleration of the material supplied from the parental circumstellar envelope and entrained by the stellar jets yielding its deceleration. Possible periodic variations of the maser emission, reflecting properties of the central dying stars or binary systems, will be further investigated.