Published June 30, 1988
| Version v1
Journal article
Do massive black holes reside in elliptical galaxies?
Creators
- 1. Cambridge Univ. (UK). Inst. of Astronomy
- 2. Massachusetts Inst. of Tech., Cambridge (USA). Center for Space Research
Description
Evidence that radio-loud quasars and powerful radio galaxies occur in elliptical galaxies suggests that most bright ellipticals now contain a 'dead' or inactive quasar. In most theories, the central 'engine' is a massive, perhaps rapidly spinning black hole, with a mass ∼ 108 - 109 M solar mass. There have been a number of searches for the massive black holes that are expected to reside at the centres of elliptical galaxies. Here we examine the accretion by a central black hole of the hot interstellar medium in an elliptical galaxy, and estimate the minimum expected luminosity and the manner of its emission. It is not obviously detected at any wavelength. (author)
Additional details
Publishing Information
- Journal Title
- Nature (London)
- Journal Volume
- 333
- Journal Issue
- 6176
- Series
- Nature (London).
- Journal Page Range
- 829-831
- ISSN
- 0028-0836
- CODEN
- NATUA
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- United Kingdom
- INIS RN
- 19086311
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Numerical Data
- Descriptors DEI
- BLACK HOLES; COSMIC GASES; ELLIPTICAL CONFIGURATION; EMISSION; GALAXIES; INTERSTELLAR SPACE; LUMINOSITY; MASS; QUASARS; THEORETICAL DATA
- Descriptors DEC
- CONFIGURATION; COSMIC RADIO SOURCES; DATA; FLUIDS; GASES; INFORMATION; NUMERICAL DATA; OPTICAL PROPERTIES; PHYSICAL PROPERTIES; SPACE