Published 1983
| Version v1
Book
Global stability analysis of an S0 galaxy NGC 3115
Creators
- 1. Tokyo Univ., Mitaka (Japan). Tokyo Astronomical Observatory
- 2. Tokyo Univ. (Japan). Dept. of Astronomy
Description
The global modal analysis is applied to a family of models which are consistent with recent dynamical data of NGC 3115. A halo component at least as massive as the disk component is required to explain the apparent lack of spiral structures in NGC 3115. (orig.)
Additional details
Publishing Information
- Publisher
- D. Reidel.
- Imprint Place
- Dordrecht (Netherlands)
- ISBN
- 90-277-1546-7
- Imprint Title
- Internal kinematics and dynamics of galaxies
- Imprint Pagination
- 432 p.
- Journal Page Range
- p. 125-126.
Conference
- Title
- International Astronomical Union symposium no. 100 on internal kinematics and dynamics of galaxies.
- Dates
- 9-13 Aug 1982.
- Place
- Besancon (France).
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- Netherlands
- INIS RN
- 15054662
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- DYNAMICS; GALAXIES; LIMITING VALUES; MASS; OSCILLATION MODES; SHAPE; STABILITY
- Descriptors DEC
- MECHANICS
Optional Information
- Notes
- short communication with 3 figs. Imprint:Includes subject, object and author index.