Candidates for Optical Counterpart in the Field of PSR 1821-24 in M28

Details Candidates for Optical Counterpart in the Field of PSR 1821-24 in M28 Candidates for Optical Counterpart in the Field of PSR 1821-24 in M28

May 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000iaus..195..431s&link_type=abstract

Highly Energetic Physical Processes and Mechanisms for Emission from Astrophysical Plasmas, Proceedings of IAU Symposium #195, h

Astronomy and Astrophysics

Astrophysics

Scientific paper

The 3-ms, X-ray pulsar RX J1824.2-2R52P has been identified at the 2-sigma level as a possible X-ray counterpart of the radio pulsar PSR 1821-24. The present work uses archival HST data for M28 to set upper limits on the optical V-band magnitude of PSR 1821-24 / RX J1824.2-2R452P. The optical limit extends the multiwavelength observations for this source and would provide constraints for theoretical models of pulsar emission.

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