Resolving Embedded X-Ray Objects in Rho OPH Cloud Core

Details Resolving Embedded X-Ray Objects in Rho OPH Cloud Core Resolving Embedded X-Ray Objects in Rho OPH Cloud Core

Sep 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999cxo..prop..137k&link_type=abstract

Chandra Proposal ID #01200705

Other

Chandra Proposal Id #01200705

Scientific paper

With the ASCA observations of the Rho Oph dark cloud, we found variable hard X-ray emission from Class I sources. A Class I (EL29) shows a flare like TTSs, other (WL6) varies sinusoidally, suggesting rotation period, and the other (YLW15) exhibit quasi-periodic flares, suggestive for the star-disk magnetic connection. Non X-ray emitting Class I is also found. Our proposal is, with no source confusion problem, to confirm these variety of X-ray activity, to search for X-rays from other Class Is, as well as new X-ray emitting young stellar objects, using ACIS with the high spatial resolution up to 10 keV energy. Together with the radio search of bipolar structure, and comparison of TTSs, our goal is to give strong constrain on the evolution and structure of protostars.

Affiliated with

Also associated with

No associations

Rating

Resolving Embedded X-Ray Objects in Rho OPH Cloud Core does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Resolving Embedded X-Ray Objects in Rho OPH Cloud Core, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Resolving Embedded X-Ray Objects in Rho OPH Cloud Core will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1553646