Colliding Wind Emission in the Runaway Binary HD 14633

Details Colliding Wind Emission in the Runaway Binary HD 14633 Colliding Wind Emission in the Runaway Binary HD 14633

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008xmm..prop...92m&link_type=abstract

XMM-Newton Proposal ID #06035702

Astronomy and Astrophysics

Astronomy

Stars, White Dwarfs, Solar System, Hd 14633, Hd 14633

Scientific paper

The runaway O-type binary HD 14633 was likely ejected from the cluster of its birth by dynamical interactions in the dense environment. Recent XMM-Newton observations have detected a soft, nonthermal X-ray flux that likely originates in a colliding wind shock region in the binary. The large variation in system separation between periastron and apastron will contribute to X-ray flux and spectral variability during the orbit. We propose observations with XMM-Newton that will measure the variable intra-system absorption, probe the geometry and physical parameters of the wind shock region, and investigate abundance anomalies in the HD 14633 binary system.

Affiliated with

Also associated with

No associations

Rating

Colliding Wind Emission in the Runaway Binary HD 14633 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 Colliding Wind Emission in the Runaway Binary HD 14633, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Colliding Wind Emission in the Runaway Binary HD 14633 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-866196