Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ap%26ss..85..231d&link_type=abstract
Astrophysics and Space Science, vol. 85, no. 1-2, July 1982, p. 231-241.
Astronomy and Astrophysics
Astronomy
1
Active Galactic Nuclei, Globular Clusters, Gravitational Waves, Pulsed Radiation, Black Holes (Astronomy), Radiation Sources, Scattering, Stellar Evolution
Scientific paper
The characteristics of gravitational bursts from active galactic nuclei and globular clusters are obtained for three astrophysical situations: (1) scattering of stars by massive black holes residued at the centers of galaxies and globular clusters; (2) the close encounters of stars in the nuclear regions of these objects; and (3) scattering of stars by black holes of stellar mass containing in the stellar population of galactic nuclei and clusters. The most effective source of gravitational bursts appears to be a scattering of stars by the massive central black holes which produces the bursts with dimensionless amplitude h = 10 to the -19th to 10 to the -21st and frequencies from 0.1 to 0.00001 Hz. The characteristics obtained correspond to the possibilities of a future gravitational-wave experiment with use of laser Doppler tracking of interplanetary spacecraft.
Dymnikova I. G.
Popov Alexander K.
Zentsova Anna S.
No associations
LandOfFree
Bursts of gravitational radiation from active galactic nuclei and globular clusters does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Bursts of gravitational radiation from active galactic nuclei and globular clusters, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Bursts of gravitational radiation from active galactic nuclei and globular clusters will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1022468