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Early stage of star formation in Orion KL

Published online by Cambridge University Press:  21 March 2013

Leonid I. Matveyenko ,
Stanislav S. Sivakon ,
Vasily A. Demichev ,
David A. Graham ,
Phillip J. Diamond  and
Martin G. Abrahamyan
Leonid I. Matveyenko
Affiliation:
IKI, 117997, Profsojuznaja 84/32, Moscow, Russia email: lmatveenko@gmail.com
Stanislav S. Sivakon
Affiliation:
IKI, 117997, Profsojuznaja 84/32, Moscow, Russia email: lmatveenko@gmail.com
Vasily A. Demichev
Affiliation:
IKI, 117997, Profsojuznaja 84/32, Moscow, Russia email: lmatveenko@gmail.com
David A. Graham
Affiliation:
MPIfR, Bonn, Germany
Phillip J. Diamond
Affiliation:
JB Observatory, UK
Martin G. Abrahamyan
Affiliation:
Erevan University, Armenia
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Abstract

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Super H2O outbursts accompany star formation. We have been studying this phenomenon in Orion KL starting in 1971.8.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S292: Molecular Gas, Dust, and Star Formation in Galaxies , August 2012 , pp. 51
Copyright
Copyright © International Astronomical Union 2013

References

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Matveenko, L. I., Zaharin, K. M., Diamond, P. J., & Graham, D. A. 2004, Astron. Reports, 2, 100Google Scholar
Demichev, V. A. & Matveenko, L. I. 2004, Astron. Reports, 12, 979Google Scholar
Matveenko, L. I. & Sivakon, S. S. 2008, Astron. Letters, 12, 820CrossRefGoogle Scholar
Matveenko, L. I. & Demichev, V. A. 2010, Astron. Letters, 11, 986Google Scholar