A very rapidly expanding gas in the core of the X-ray globular cluster NGC 6624

Details A very rapidly expanding gas in the core of the X-ray globular cluster NGC 6624 A very rapidly expanding gas in the core of the X-ray globular cluster NGC 6624

Apr 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980esasp.157..183b&link_type=abstract

The second European International Ultraviolet Explorer (IUE) Conference, held 26-28 March 1980 in Tübingen, West Germany. Edited

Astronomy and Astrophysics

Astronomy

2

Globular Clusters, Iue, Ultraviolet Astronomy, X Ray Sources, Carbon, Doppler Effect, Emission Spectra, Nitrogen, Silicon

Scientific paper

International Ultraviolet Explorer observations of the center of the
X-ray globular cluster NGC 6624 reveal an emission line spectrum. A
tentative identification needs a very large velocity of 10,000 km/sec. A
point source emits most of the UV flux with a continuum distribution. A
resolved expanding nebula would emit the emission line spectrum.

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