e-Article
A high-frequency radio observation of NGC 6624
Document Type
Report
Source
Astronomy and Astrophysics. 280(2)
Subject
Language
English
ISSN
0004-6361
Abstract
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.