X-ray and Radio Imaging of the Protostar Complex Adjacent to IC 348

Details X-ray and Radio Imaging of the Protostar Complex Adjacent to IC 348 X-ray and Radio Imaging of the Protostar Complex Adjacent to IC 348

Sep 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007cxo..prop.2343w&link_type=abstract

Chandra Proposal ID #09200564

Physics

Chandra Proposal Id #09200564

Scientific paper

Among several classes of active stars and solar flares, a tight relation between X-ray and radio luminosities is found. This relation implies an intimate physical connection. We propose a pair of 40 ks coordinated VLA/ACIS-I observations of a newly revealed filamentary structure of nearly two dozen protostars and pre-stellar cores just southwest of IC 348. Using extant Spitzer and SCUBA data we have a full inventory of the stellar types in this cluster which contains Class 0 and Class I protostars and outflow sources in addition to classical and weak T-Tauri stars. We will complete the census of this nearby, actively forming, sub-cluster and study the causal relation of radio and X-ray emission for all types of young stars, both in flare and quiescent.

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