Published June 30, 1988 | Version v1
Journal article

Do massive black holes reside in elliptical galaxies?

  • 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