Abstract
The region(s) within the magnetosphere where the IR -- UV emissions arise is essentially unknown. This work is an attempt to place constraints on possible emission regions using a computationally intensive, inverse mapping approach. This approach can yield a localisation of emission regions within the magnetosphere and also gives an estimate of pulsar inclination angles. Initial results for PSR B0531+21 (the Crab) are presented.
Original language | English (Ireland) |
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Title of host publication | RELATIVISTIC ASTROPHYSICS |
Publication status | Published - 1 Jan 2001 |
Authors (Note for portal: view the doc link for the full list of authors)
- Authors
- O'Connor, P,Shearer, A,Golden, A,Eikenberry, S,Wheeler, JC,Martel, H