Published July 1985
| Version v1
Journal article
Decay dynamics of nonstationary open clusters
Description
Computer simulation of the dynamics of nonisolated open clusters indicates, on the basis of a model halo zone expanding as weak stellar encounters relax the system, that member stars will intensively escape into the galactic force field. The old clusters M67 and NGC 188 are still far from a steady state
Additional details
Publishing Information
- Journal Title
- Sov. Astron. (Engl. Transl.)
- Journal Volume
- 29
- Journal Issue
- 4
- Series
- Sov. Astron. (Engl. Transl.).
- Journal Page Range
- 413-417
- ISSN
- 0038-5301
- CODEN
- SAAJA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 17048864
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- COMPUTERIZED SIMULATION; DYNAMICS; EXPANSION; GRAVITATIONAL FIELDS; MILKY WAY; MOTION; STABILITY; STAR CLUSTERS; STAR EVOLUTION
- Descriptors DEC
- GALAXIES; MECHANICS; SIMULATION
Optional Information
- Notes
- Cover-to-cover translation of Astronomicheskij Zhurnal (USSR).