Limits on the optical magnitude of PSR 1821-24 in M28

Details Limits on the optical magnitude of PSR 1821-24 in M28 Limits on the optical magnitude of PSR 1821-24 in M28

2000-04-14

arxiv.org/abs/astro-ph/0004198v1

Pulsar Astronomy - 2000 and Beyond, ASP Conference Series, Vol. 202; Proceedings of the 177th Colloquium of the IAU held in Bo

Astronomy and Astrophysics

Astrophysics

Two pages, two figures, in press. Please email any questions/comments to fks@iucaa.ernet.in

Scientific paper

The detection of a pulsed X-ray counterpart (RX J1824.2-2R52P) of the 3.05 ms pulsar PSR 1821-24, suggests the possibility of a part of the rotational energy loss of this high spindown rate pulsar being in the optical band. Archival HST data for M28 is used here to set upper limits on the optical V-band magnitude of PSR 1821-24. The optical limit extends the multiwavelength observations for this source and provides a constraint for theoretical models of pulsar emission.

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