Results from DROXO: III. Observation, source list, and X-ray properties of sources detected in the "deep Rho Ophiuchi XMM-Newton Observation"

Astronomy and Astrophysics

Volumn 519, Issue 3, 2010, Pages

  Pillitteri, I ^a,b,i   Sciortino, S ^b   Flaccomio, E ^b   Stelzer, B ^b   Micela, G ^b   Damiani, F ^b   Testi, L ^c   Montmerle, T ^d   Grosso, N ^e,f   Favata, F ^g   Giardino, G ^h  

^a UNIVERSITY OF PALERMO   (Italy)

^b INAF OSSERVATORIO ASTROFISICO DI TORINO   (Italy)

^c EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^d UNIV GRENOBLE ALPES   (France)

^e UNIVERSITÉ DE STRASBOURG   (France)

^f CNRS   (France)

^g EUROPEAN SPACE AGENCY   (France)

^h EUROPEAN SPACE AGENCY   (Netherlands)

ⁱ HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

Author keywords

Galaxy: formation; stars: coronae; stars: formation; X rays: stars

Indexed keywords

ABSORPTION SPECTROSCOPY; ELECTROMAGNETIC WAVE EMISSION; GALAXIES; ION BEAMS; X RAY SCATTERING; X RAYS;

CIRCUMSTELLAR MATERIALS; CLASS I; CLASS II; DETECTION RATES; GALAXY: FORMATION; INFRARED OBSERVATIONS; LARGE PROGRAMS; LIGHT CURVES; ORION NEBULA; PLASMA TEMPERATURE; SIGNAL TO NOISE; SOFT COMPONENTS; SPITZER; STAR FORMATIONS; STARS: CORONAE; STARS: FORMATION; THERMAL COMPONENT; X RAY SPECTRUM; X RAYS: STARS; X-RAY EMISSION; X-RAY PROPERTIES; XMM-NEWTON; XMM-NEWTON OBSERVATIONS; YOUNG STARS; YOUNG STELLAR OBJECTS;

STARS;

EID: 77956497647     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200911873     Document Type: Article

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