What can we learn from Neutron Star X-Ray Binaries' JETS?

Details What can we learn from Neutron Star X-Ray Binaries' JETS? What can we learn from Neutron Star X-Ray Binaries' JETS?

Nov 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ap%26ss.300..197m&link_type=abstract

Astrophysics and Space Science, Volume 300, Issue 1-3, pp. 197-209

Astronomy and Astrophysics

Astrophysics

Binaries, Close, Stars, Jets And Outflows, Radio Continuum

Scientific paper

We review our current knowledge of the disk-jet coupling in neutron star X-ray binaries. We compare neutron star and black hole X-ray binaries, by means of radio and X-ray observations, in order to understand the role played in the production of the jet, by characteristics proper of the accreting compact object involved: the existence of a solid surface, the presence of an ergosphere/event horizon, the strength of the magnetic field, the spin of the compact object.

Affiliated with

Also associated with

No associations

Rating

What can we learn from Neutron Star X-Ray Binaries' JETS? 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 What can we learn from Neutron Star X-Ray Binaries' JETS?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and What can we learn from Neutron Star X-Ray Binaries' JETS? will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1835148