Joint Discussion 2 On the present and future of pulsar astronomy

Details Joint Discussion 2 On the present and future of pulsar astronomy Joint Discussion 2 On the present and future of pulsar astronomy

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007hia....14..109b&link_type=abstract

Highlights of Astronomy, Volume 14, p. 109-138

Astronomy and Astrophysics

Astronomy

Scientific paper

Neutron stars are formed in supernova explosions. They manifest themselves in many different ways, for example, as pulsars, anomalous X-ray pulsars (AXPs) and soft γ-ray repeaters (SGRs) and the so-called ‘radio-quiet neutron stars’. These objects are made visible by high-energy processes occurring on their surface or in the surrounding region. In most of these objects, ultra-strong magnetic fields are a crucial element in the radio, optical, X-ray and gamma-ray emission processes which dominate the observed spectrum.

Affiliated with

Also associated with

No associations

Rating

Joint Discussion 2 On the present and future of pulsar astronomy 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 Joint Discussion 2 On the present and future of pulsar astronomy, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Joint Discussion 2 On the present and future of pulsar astronomy will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-974540