Published November 1982
| Version v1
Journal article
H2O maser flare in Orion A
Creators
- 1. Institute for Space Research, USSR Academy of Sciences, Moscow, USSR
Description
The flare of H2O maser emission in Orion A was observed with the Crimea--Effelsberg and Haystack--Green Bank interferometers in November 1979. Its position is α = 5/sup h/32/sup m/46/sup s/.6 +- 0/sup s/.06, delta = -5024'.28''.7 +- 1'' (1950.0); its radial velocity, 8 km/sec. The asymmetric line profile has a 28-kHz halfwidth. The flare source comprises a 0''.0005 core (T/sub b/ = 5 x 10160K) embedded in a 0''.005 halo (T/sub b/ = 3 x 10140K)
Additional details
Publishing Information
- Journal Title
- Sov. Astron. Lett. (Engl. Transl.)
- Journal Volume
- 8
- Journal Issue
- 6
- Series
- Sov. Astron. Lett. (Engl. Transl.).
- Journal Page Range
- 382-383
- ISSN
- 0360-0327
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 14790338
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- COORDINATES; COSMIC GASES; COSMOCHEMISTRY; EMISSION SPECTRA; GHZ RANGE 01-100; INTERFEROMETRY; MASERS; MICROWAVE RADIATION; NEBULAE; RADIAL VELOCITY; WATER
- Descriptors DEC
- AMPLIFIERS; CHEMISTRY; ELECTROMAGNETIC RADIATION; ELECTRONIC EQUIPMENT; EQUIPMENT; FLUIDS; FREQUENCY RANGE; GASES; GHZ RANGE; HYDROGEN COMPOUNDS; MICROWAVE AMPLIFIERS; MICROWAVE EQUIPMENT; OXYGEN COMPOUNDS; RADIATIONS; SPECTRA; VELOCITY
Optional Information
- Notes
- Cover-to-cover translation of Pis'ma v Astronomicheskij Zhurnal (USSR).