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A flare of the H2O maser in the source Orion KL

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Abstract

In 1998, the intensity of the 1.35-cm H2O maser radio line in the source Orion KL increased several hundreds of times. The observations of this flare and its behavior with time are presented.

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References

  1. G. Garay, J. M. Moran, and A. D. Haschick, Astrophys. J. 338, 244 (1989).

    Article  ADS  Google Scholar 

  2. R. A. Gaume, T. L. Wilson, R. J. Vrba, et al., Astrophys. J. 493, 940 (1998).

    Article  ADS  Google Scholar 

  3. L. I. Matveenko, Pis'ma Astron. Zh. 20, 456 (1994) [Astron. Lett. 20, 388 (1994)].

    ADS  Google Scholar 

  4. Z. Abraham, and J. W. S. Vilas Boas, Astron. Astrophys. 290, 956 (1994).

    ADS  Google Scholar 

  5. L. I. Matveenko, P. D. Daimond, and D. A. Graham, Pis'ma Astron. Zh. 24, 723 (1998) [Astron. Lett. 24, 623 (1998)].

    ADS  Google Scholar 

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Authors and Affiliations

  1. Pushchino Radio Astronomy Observatory, Astrospace Center, Lebedev Physical Institute, Russian Academy of Sciences, Pushchino, Moscow oblast, 142292, Russia

    A. M. Tolmachev

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  1. A. M. Tolmachev
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Translated from Pis'ma v Astronomicheski\(\overset{\lower0.5em\hbox{$\smash{\scriptscriptstyle\smile}$}}{l} \) Zhurnal, Vol. 26, No. 1, 2000, pp. 41–44.

Original Russian Text Copyright © 2000 by Tolmachev.

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Tolmachev, A.M. A flare of the H2O maser in the source Orion KL. Astron. Lett. 26, 34–37 (2000). https://doi.org/10.1134/1.20366

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  • DOI: https://doi.org/10.1134/1.20366

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