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Brightness temperatures of galactic masers observed in the RadioAstron project

Published online by Cambridge University Press:  16 July 2018

Nadezhda N. Shakhvorostova ,
Alexey V. Alakoz  and
Andrej M. Sobolev
Nadezhda N. Shakhvorostova
Affiliation:
Astro-Space Center of Lebedev Physical Institute, 84/32 Profsoyuznaya st., Moscow, GSP-7, 117997, Russia, email: nadya@asc.rssi.ru, alexey.alakoz@gmail.com
Alexey V. Alakoz
Affiliation:
Astro-Space Center of Lebedev Physical Institute, 84/32 Profsoyuznaya st., Moscow, GSP-7, 117997, Russia, email: nadya@asc.rssi.ru, alexey.alakoz@gmail.com
Andrej M. Sobolev
Affiliation:
Ural Federal University, 19 Mira street, Ekaterinburg, 620002, Russia email: Andrej.Sobolev@urfu.ru
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Abstract

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We present estimates of brightness temperature for 5 galactic masers in star-forming regions detected at space baselines. Very compact features with angular sizes of ~23-60 μas were detected in these regions with corresponding linear sizes of ~4-10×106 km. Brightness temperatures range from 1014 up to 1016 K.

Keywords

maserstechniques: high angular resolution
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 13 , Symposium S336: Astrophysical Masers: Unlocking the Mysteries of the Universe , September 2017 , pp. 447 - 448
Copyright
Copyright © International Astronomical Union 2018 

References

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