Published September 1985
| Version v1
Journal article
Infrared radiation of galaxy protoclusters (pancakes) and protogalaxies
Creators
- 1. Rostovskij-na-Donu Gosudarstvennyj Univ. (USSR)
- 2. Volgogradskij Gosudarstvennyj Univ. (USSR)
Description
Characteristics of the HI and H2 IR lines of protoclusters of galaxies (''pancakes'') and young galaxies are calculated. In vibrational-rotational transitions of H2 the radiation fluxes expected from the ''pancakes'' are Fsub(ν) approximately 10-3-10-2 Jy, and in recombination lines of atomic hydrogen they make up Fsub(ν) approximately 10-5-10-4 Jy. It is possible to record from protogalaxies radiation in recombination lines of atomic hydrogen. The IR radiation in the lines of molecular hydrogen in this case is very weak, Fsub(ν) < 10-5 Jy
Additional details
Additional titles
- Original title (Russian)
- Инфракрасное излучение протоскоплений галактик (блинов) и протогалактик
Publishing Information
- Journal Title
- Astron. Zh.
- Journal Volume
- 62
- Journal Issue
- 5
- Series
- Astron. Zh.
- Journal Page Range
- 841-846
- ISSN
- 0004-6299
- CODEN
- ASZHA
INIS
- Country of Publication
- Russian Federation
- Country of Input or Organization
- USSR
- INIS RN
- 17056810
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Numerical Data
- Descriptors DEI
- ATOMS; ENERGY-LEVEL TRANSITIONS; FLUX DENSITY; GALAXIES; GALAXY CLUSTERS; HYDROGEN; H2 REGIONS; INFRARED RADIATION; MOLECULES; RADIATION FLUX; RECOMBINATION; THEORETICAL DATA
- Descriptors DEC
- COSMIC RADIO SOURCES; DATA; ELECTROMAGNETIC RADIATION; ELEMENTS; INFORMATION; NONMETALS; NUMERICAL DATA; RADIATIONS
Optional Information
- Notes
- For English translation see the journal Soviet Astronomy (USA).