Published 1989
| Version v1
Book
Dynamics of the center of M32
Description
Observations are presented of the surface brightness and rotation of the center of M32. The luminosity density is accurately described as a power law of slope -2.2 from 1-30 parsec. The projected rotation field has constant angular velocity on isophotes, and increases at small radii to an unresolved cusp at the centre with amplitude of at least 60 km/s. The internal rotation field is modelled, and the internal mean rotation must reach an amplitude of at least 90 km/s at a radius of 2 parsecs. (author)
Additional details
Publishing Information
- Publisher
- Cambridge University Press.
- Imprint Place
- Cambridge (UK)
- ISBN
- 0 521 364329
- Imprint Title
- Dynamics of dense stellar systems
- Imprint Pagination
- 251 p.
- Journal Page Range
- p. 35-41.
Conference
- Title
- Dynamics of dense stellar systems workshop.
- Dates
- 27-28 May 1988.
- Place
- Toronto (Canada).
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- United Kingdom
- INIS RN
- 21055935
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference, Numerical Data
- Descriptors DEI
- ANGULAR VELOCITY; BRIGHTNESS; DYNAMICS; EXPERIMENTAL DATA; GALAXIES; GALAXY NUCLEI; NONLUMINOUS MATTER; ROTATION; SPATIAL DISTRIBUTION; VISIBLE SPECTRA
- Descriptors DEC
- DATA; DISTRIBUTION; INFORMATION; MATTER; MECHANICS; NUMERICAL DATA; OPTICAL PROPERTIES; PHYSICAL PROPERTIES; SPECTRA; VELOCITY