Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 1978
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978stin...7910994s&link_type=abstract
"On the nature of the sources of hard pulse X-ray radiation Transl. into ENGLISH of "O Prirode Istochnikov Impulsnogo Zhestkogo
Astronomy and Astrophysics
Astronomy
Cosmic Rays, Globular Clusters, Pulsed Radiation, Stellar Radiation, X Ray Sources, Astronomical Netherlands Satellite, Black Holes (Astronomy), Cosmos Satellites, Galactic Radiation, Gamma Rays
Scientific paper
Besides the identified sources of cosmic pulse X-ray radiation with globular clusters NGC 6624, NGC 1851 and MXB 1730-335 several new identifications were made. The source in Norma was probably identified with globular cluster NGC 5927, the source in Aquila with globular cluster NGC 6838 (M71), and the source in Puppis with globular cluster NGC 2298. Gamma pulses discovered by the Vela satellites and X-ray pulses thoroughly measured by the SAS-3, Ariel-5, and ANS satellites are thought to be the same phenomenon. The sources of such a radiation must be some kind of peculiarity at the central part of globular clusters; it is most probably a massive black hole. The sources of hard pulse radiation which cannot be identified with globular clusters are considered to be a new kind of galactic object, invisible globular clusters, which are naked nuclei of globular clusters.
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