Soft X-ray to far infrared luminosities ratio in star-forming galaxies: Predictions from synthesis models

Astronomy and Astrophysics

Volumn 483, Issue 1, 2008, Pages 71-78

  Mas Hesse, J M ^a   Oti Floranes H ^a,b   Cervino M ^c  

^a CENTRO DE ASTROBIOLOGÍA CSIC INTA   (Spain)

^b UNIVERSITY OF CANTABRIA   (Spain)

^c INSTITUTO DE ASTROFÍSICA DE ANDALUCÍA CSIC   (Spain)

Author keywords

Galaxies: starburst; ISM: kinematics and dynamics; ISM: supernova remnants; X rays: galaxies; X rays: ISM

Indexed keywords

INFRARED RADIATION; MATHEMATICAL MODELS; STARS; X RAYS;

INFRARED LUMINOSITIES; STAR FORMING; SUPERNOVA REMNANTS;

GALAXIES;

EID: 43049126868     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20078398     Document Type: Article

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