Simultaneous X-ray, radio, near-infrared, and optical monitoring of young stellar objects in the Coronet cluster

Astronomy and Astrophysics

Volumn 464, Issue 3, 2007, Pages 1003-1013

  Forbrich, J ^a,b   Preibisch, Th ^a   Menten, K M ^a   Neuhauser R ^b   Walter, F M ^c   Tamura, M ^d   Matsunaga, N ^e   Kusakabe, N ^f   Nakajima, Y ^d   Brandeker, A ^g   Fornasier, S ^h   Posselt, B ^b,i   Tachihara, K ^j   Broeg, C ^b  

^a MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

^b Astrophysikalisches Institut   (Germany)

^c STONY BROOK UNIVERSITY   (United States)

^d NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^e UNIVERSITY OF TOKYO   (Japan)

^f GRADUATE UNIVERSITY FOR ADVANCED STUDIES   (Japan)

^g UNIVERSITY OF TORONTO   (Canada)

^h UNIVERSITÉ PARIS DESCARTES   (France)

ⁱ MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^j KOBE UNIVERSITY   (Japan)

more..

Author keywords

Infrared: stars; Radio continuum; Stars; Stars: individual: R CrA; Stars: individual: S CrA; Stars: pre main sequence; X rays: stars

Indexed keywords

CORRELATION METHODS; LIGHT EMISSION; OPTICAL PROPERTIES; OPTICAL TELESCOPES; STARS; X RAY ANALYSIS;

CORONAL PROCESSES; RADIO CONTINUUM; STELLAR CORONA; STELLAR SURFACE;

ASTROPHYSICS;

EID: 33947712087     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20066158     Document Type: Article

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