A possible detection of diffuse extended X-ray emission in the environment of the globular cluster NGC 6779

Details A possible detection of diffuse extended X-ray emission in the environment of the globular cluster NGC 6779 A possible detection of diffuse extended X-ray emission in the environment of the globular cluster NGC 6779

Jul 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000mnras.316l...5h&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 316, Issue 1, pp. L5-L8.

Astronomy and Astrophysics

Astronomy

5

Globular Clusters: General, Globular Clusters: Individual: Ngc 6779, X-Rays: General, X-Rays: Ism

Scientific paper

We report the possible detection of diffuse X-ray emission in the environment of NGC 6779, and find the emission to be well aligned with the proper motion of the cluster. The position of the emission suggests we are observing heated ISM in the wake of the cluster that could be the result of an interaction between the intracluster medium and the halo gas surrounding it.

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