Normal galaxies in the XMM-Newton fields X-rays as a star formation indicator

Astronomy and Astrophysics

Volumn 502, Issue 1, 2009, Pages 85-90

  Rovilos, E ^a,b,c   Georgantopoulos, I ^b   Tzanavaris, P ^b,d,e   Pracy, M ^f   Whiting, M ^g   Woods, D ^h,i   Goudis, C ^b,c  

^a MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^b NATIONAL OBSERVATORY OF ATHENS   (Greece)

^c UNIVERSITY OF PATRAS   (Greece)

^d NASA GODDARD SPACE FLIGHT CENTER   (United States)

^e JOHNS HOPKINS UNIVERSITY   (United States)

^f AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

^g CSIRO   (Australia)

^h UNIVERSITY OF NEW SOUTH WALES   (Australia)

ⁱ UNIVERSITY OF BRITISH COLUMBIA   (Canada)

Author keywords

Galaxies: Starburst; X rays: Galaxies

Indexed keywords

AUSTRALIAN NATIONAL UNIVERSITY; EMISSION LINES; EXTENDED SOURCES; GALACTIC STARS; GALAXIES: STARBURST; LATE-TYPE; RED SHIFT; STAR FORMATIONS; X-RAY EMISSION; X-RAY LUMINOSITY; X-RAYS: GALAXIES; XMM-NEWTON;

DATABASE SYSTEMS; ELECTROMAGNETIC WAVE EMISSION; EMISSION SPECTROSCOPY; GALAXIES; LIGHT TRANSMISSION; LUMINANCE;

X RAYS;

EID: 68349104217     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912053     Document Type: Article

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