Published April 1980
| Version v1
Journal article
Spectroscopic investigation of the VV 126 multicomponent interacting system
Creators
- 1. Moskovskij Gosudarstvennyj Univ. (USSR). Gosudarstvennyj Astronomicheskij Inst. ''GAISh''
Description
The object VV 126 was investigated using spectrograms obtained with the 6-m telescope. VV 126 is a system of two or more distorted giant galaxies with peculiar velocity field. The system contains emission knots, which are gian H2 regions - superassociations. If the system is stable, its total mass is approximately 1011 Msub(sun). Relative intensities of emission lines are similar to those observed for H2 regions in spiral structure of ordinary galaxies
Additional details
Additional titles
- Original title (Russian)
- Спектроскопическое исследование многокомпонентной взаимодействующей системы VV 126
Publishing Information
- Journal Title
- Pis'ma Astron. Zh.
- Journal Volume
- 6
- Journal Issue
- 4
- Series
- Pis'ma Astron. Zh.
- Journal Page Range
- 202-207
- ISSN
- 0320-0108
INIS
- Country of Publication
- Russian Federation
- Country of Input or Organization
- USSR
- INIS RN
- 11563710
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- EMISSION SPECTRA; GALAXIES; H2 REGIONS; LIMITING VALUES; LINE WIDTHS; MASS; RADIAL VELOCITY; SPECTROPHOTOMETRY; VISIBLE RADIATION
- Descriptors DEC
- COSMIC RADIO SOURCES; ELECTROMAGNETIC RADIATION; RADIATIONS; SPECTRA; VELOCITY
Optional Information
- Notes
- For English translation see the journal Soviet Astronomy Letters (USA).