An unusual discontinuity in the X-ray surface brightness profile of NGC 507: Evidence of an abundance gradient?

Astrophysical Journal

Volumn 601, Issue 1 I, 2004, Pages 221-227

  Kraft, R P ^a   Forman, W R ^a   Churazov, E ^b,c   Laslo, N ^a   Jones, C ^a   Markevitch, M ^a   Murray, S S ^a   Vikhlinin, A ^a  

^a HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^b MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^c Space Research Institute ^*  (Russian Federation)

Author keywords

Galaxies: individual (NGC 507); Galaxies: ISM; X rays: galaxies

Indexed keywords

EID: 1642617900     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/380427     Document Type: Article

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