Analysis of the spectral energy distribution from a runaway star bow shock

Details Analysis of the spectral energy distribution from a runaway star bow shock Analysis of the spectral energy distribution from a runaway star bow shock

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011rmxac..40..156p&link_type=abstract

XIII Latin American Regional IAU Meeting (Eds. W. J. Henney & S. Torres-Peimbert) Revista Mexicana de Astronomía y Astrofísica (

Astronomy and Astrophysics

Astronomy

Scientific paper

The bow shock produced by the high-mass runaway star BD +43° 3654 (Comerón & Pasquali 2007) has been detected as a non-thermal radio source (S_ν ∝ ν^{-α}, <α>=0.5) and it is the first one of that type ever observed (Benaglia et al. 2010). The non-thermal detection provides evidence of the presence of a magnetic field and relativistic electrons. This population of relativistic particles can produce high-energy (HE) emission.

Affiliated with

Also associated with

No associations

Rating

Analysis of the spectral energy distribution from a runaway star bow shock 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 Analysis of the spectral energy distribution from a runaway star bow shock, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Analysis of the spectral energy distribution from a runaway star bow shock will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1674200