Physics
Scientific paper
Jul 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005sfet.confe..40f&link_type=abstract
"Star Formation in the Era of Three Great Observatories, meeting abstracts from the conference held July 13-15, 2005 in Cambridg
Physics
Scientific paper
The Coronet Cluster in the nearby R CrA dark cloud offers the rare opportunity to study a sample of at least four ``class I'' protostars as well as one class 0 source plus a Herbig Ae star within a few arcminutes at a distance of only 150 pc. Most of these sources are detected at radio, X-ray, and infrared wavelengths and present a diverse view in radio and X-ray data we report here. We analyzed multi-epoch Very Large Array (VLA) as well as archival Chandra and XMM-Newton data taken in 1998 and 2000-2003, respectively. Upcoming simultaneous multi-wavelength radio, X-ray, and near-infrared observations will offer the possibility to study interconnections and lead to conclusions concerning the underlying physics. For example, correlations of the variability in hard X-ray and centimetric radio emission from these sources could lead to new insights into their coronal processes, while correlations between lower-energy X-ray and infrared emission could probe accretion activity.
Forbrich Jan
Menten Karl
Preibisch Thomas
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