Observations of X rays from near NGC6440

Details Observations of X rays from near NGC6440 Observations of X rays from near NGC6440

Sep 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975natur.257...32m&link_type=abstract

Nature, vol. 257, Sept. 4, 1975, p. 32, 33.

Astronomy and Astrophysics

Astronomy

47

Globular Clusters, Satellite Observation, Spaceborne Astronomy, X Ray Sources, Galactic Nuclei, Oso-7, Radiant Flux Density, X Ray Astronomy

Scientific paper

Analysis of all-sky maps made by OSO-7 during scanning of the region within about 10 deg of galactic center has led to the discovery of X-ray sources near the globular cluster NGC6440. The most intense of these, MX1746-60, is highly variable on time scales of months. Its counterpart, NGC6440, is concentrated, supporting theories of globular cluster X-ray emission requiring high central densities to encourage formation of binary systems. X-ray flux data for MX1746-60 are given.

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