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

Monthly Notices of the Royal Astronomical Society

Volumn 316, Issue 1, 2000, Pages

  Hopwood, M E L ^a   Evans, A ^a   Roberts, T P ^b   Burleigh, M R ^b   Odenkirchen, M ^c   Beardmore, A P ^a   O'Brien, T ^d   Jeffries, R D ^a   Penny, A ^e   Eyres, S P S ^a,f  

^a KEELE UNIVERSITY   (United Kingdom)

^b UNIVERSITY OF LEICESTER   (United Kingdom)

^c CNRS   (France)

^d UNIVERSITY OF MANCHESTER   (United Kingdom)

^e RUTHERFORD APPLETON LABORATORY   (United Kingdom)

^f Twelve Quays House   (United Kingdom)

Author keywords

Globular clusters: general; Globular clusters: individual: NGC 6779; X rays: general; X rays: ISM

Indexed keywords

ELECTROMAGNETIC WAVE EMISSION; GALAXIES;

GLOBULAR CLUSTER: INDIVIDUAL: NGC 6779; GLOBULAR CLUSTERS; GLOBULAR CLUSTERS: INDIVIDUAL; GLOBULAR CLUSTERS:GENERAL; INTRACLUSTER MEDIUM; PROPER MOTION; X RAYS: ISM; X-RAY EMISSION; X-RAY GENERAL;

X RAY SCATTERING;

EID: 0040892365     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2000.03717.x     Document Type: Article

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