A high-frequency radio observation of NGC 6624

Details A high-frequency radio observation of NGC 6624 A high-frequency radio observation of NGC 6624

Dec 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...280..523j&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 280, no. 2, p. 523-524

Astronomy and Astrophysics

Astronomy

3

Globular Clusters, Pulsars, Radio Astronomy, Radio Observation, Angular Resolution, Very Large Array (Vla), X Ray Binaries

Scientific paper

We report a high-frequency Very Large Array (VLA) observation of the
globular cluster NGC 6624. No source is detected at 8 GHz, which implies
that the radio source seen at 1.4 GHz (Johnston & Kulkarni 1992) is
in fact one of the pulsars, and not the X-ray binary.

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