Abstract
If Weber's gravitational-wave observations are interpreted in terms of a source at the Galactic center, both the intensity and the frequency of the waves are more reasonable if the source is assumed to emit in a synchrotron mode (narrow angles, high harmonics). Although presently studied sources for such modes are astrophysically unsatisfactory—high-energy, nearly circular, scattering orbits—other possible sources are under study.
- Received 22 November 1971
DOI:https://doi.org/10.1103/PhysRevLett.28.994
©1972 American Physical Society
