Published April 1, 1984 | Version v1
Journal article Metadata-only

Gravitational waves from a population of binary black holes

Creators

  • 1. Stanford Univ., CA (USA). Dept. of Physics
  • 2. Cambridge Univ. (UK). Inst. of Astronomy
  • 3. Kyoto Univ. (Japan). Research Inst. for Fundamental Physics

Description

Arguments are presented for believing that a large fraction of the 'missing mass' may be in binary black hole remnants of population III stars with mass M exceeding 102 solar masses. The characteristics of the gravitational waves which would be generated by these binaries are discussed. (author)

Additional details

Publishing Information

Journal Title
Mon. Not. R. Astron. Soc.
Journal Volume
207
Journal Issue
3
Series
Mon. Not. R. Astron. Soc.
Journal Page Range
585-609
ISSN
0035-8711

INIS

Country of Publication
United Kingdom
Country of Input or Organization
United Kingdom
INIS RN
15054743
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
BINARY STARS; BLACK HOLES; COALESCENCE; GRAVITATIONAL RADIATION; GRAVITATIONAL WAVES; MATHEMATICAL MODELS; MISSING MASS
Descriptors DEC
MASS; RADIATIONS; STARS