Published October 1987
| Version v1
Journal article
Flare of H2O maser radiation-protoplanetary rings
Creators
Description
Maser radiation flare in the Orion nebula is investigated. Observations made by the Simenz-Effelsberg-Opsala radiointerference net in 1982 permitted to single out several compact components in the region of the flare, which form a chain. The chain of components corresponds to concentric rings. High degree of linear polarization of the maser source is explained by magnetic field of the rings. Expanding rings must have different position angles of the polarization plane
Additional details
Additional titles
- Original title (Russian)
- Вспышка мазерного излучения Х
Publishing Information
- Journal Title
- Astron. Vestn.
- Journal Volume
- 21
- Journal Issue
- 4
- Series
- Astron. Vestn.
- Journal Page Range
- 308-311
- ISSN
- 0320-930X
- CODEN
- ASVEA
Conference
- Title
- Astrophysical problems of the planetary cosmology.
- Dates
- 1 Apr 1987.
- Place
- Moscow (USSR).
INIS
- Country of Publication
- Russian Federation
- Country of Input or Organization
- USSR
- INIS RN
- 19102534
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- H2 REGIONS; POLARIZATION; PROTOPLANETS; RINGS; STIMULATED EMISSION; WATER VAPOR
- Descriptors DEC
- COSMIC RADIO SOURCES; EMISSION; ENERGY-LEVEL TRANSITIONS; FLUIDS; GASES; VAPORS