Iron fluorescent line emission from young stellar objects in the Orion Nebula

Astrophysical Journal, Supplement Series

Volumn 160, Issue 2, 2005, Pages 503-510

  Tsujimoto, M ^a   Feigelson, E D ^a   Grosso, N ^b   Micela, G ^c   Tsuboi, Y ^d   Favata, F ^e   Shang, H ^f   Kastner, J H ^g  

^a PENNSYLVANIA STATE UNIVERSITY   (United States)

^b UNIV GRENOBLE ALPES   (France)

^c INAF OSSERVATORIO ASTROFISICO DI TORINO   (Italy)

^d CHUO UNIVERSITY   (Japan)

^e EUROPEAN SPACE AGENCY   (Netherlands)

^f INSTITUTE OF ASTRONOMY AND ASTROPHYSICS   (Taiwan)

^g ROCHESTER INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

ISM: individual (OMC 1); Open clusters and associations: individual (Orion Nebula Cluster)scattering stars: pre main sequence; X rays: stars

Indexed keywords

EID: 27644563468     PISSN: 00670049     EISSN: None     Source Type: Journal    
DOI: 10.1086/432093     Document Type: Article

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