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

Published online by Cambridge University Press:  25 May 2016

F. K. Sutaria
F. K. Sutaria*
Affiliation:
Inter-University Centre for Astronomy and Astrophysics, Pune, India

Abstract

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The 3-ms, X-ray pulsar RX J1824.2-2R52P has been identified at the 2-σ 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.

Type
Part II: Posters
Information
Symposium - International Astronomical Union , Volume 195: Highly Energetic Physical Processes and Mechanisms , 2000 , pp. 431 - 432
Copyright
Copyright © Astronomical Society of the Pacific 2000 

References

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