Inverse mapping of non thermal optical emission from isolated neutron stars: 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.

Aaron Golden

Inverse mapping of non thermal optical emission from isolated neutron stars: 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.

Physics

Research output: Contribution to conference (Published) › Abstract

Original language	English (Ireland)
Publication status	Published - 1 Jan 2000
Event	20th Texas Symposium on relativistic astrophysics. 2000 - Duration: 11 Dec 2000 → …

Conference

Conference	20th Texas Symposium on relativistic astrophysics. 2000
Period	11/12/00 → …

Authors (Note for portal: view the doc link for the full list of authors)

Authors
O'Connor, P;Shearer, A;Golden, A;Eikenberry, S

Cite this

Golden, A. (2000). Inverse mapping of non thermal optical emission from isolated neutron stars: 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.. Abstract from 20th Texas Symposium on relativistic astrophysics. 2000.

Golden, Aaron. / Inverse mapping of non thermal optical emission from isolated neutron stars : 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. Abstract from 20th Texas Symposium on relativistic astrophysics. 2000.

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title = "Inverse mapping of non thermal optical emission from isolated neutron stars: 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.",

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Golden, A 2000, 'Inverse mapping of non thermal optical emission from isolated neutron stars: 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.', 20th Texas Symposium on relativistic astrophysics. 2000, 11/12/00.

Inverse mapping of non thermal optical emission from isolated neutron stars: 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. / Golden, Aaron.
2000. Abstract from 20th Texas Symposium on relativistic astrophysics. 2000.

Research output: Contribution to conference (Published) › Abstract

Golden A. Inverse mapping of non thermal optical emission from isolated neutron stars: 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.. 2000. Abstract from 20th Texas Symposium on relativistic astrophysics. 2000.