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Hubble Space Telescope Proper Motion Confirms the Optical Identification of the Nearby Pulsar PSR 1929+10*

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Published 2002 October 28 © 2002. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Roberto P. Mignani et al 2002 ApJ 580 L147 DOI 10.1086/345291

1538-4357/580/2/L147

Abstract

We report on the proper-motion measurement of the proposed optical counterpart of the X-ray/radio pulsar PSR 1929+10. Using images obtained with the Hubble Space Telescope (HST) Space Telescope Imaging Spectrograph (STIS; average epoch 2001.73), we computed a yearly displacement of +97 ± 1 mas yr-1 in right ascension and +46 ± 1 mas yr-1 in declination since the epoch (1994.52) of the original HST Faint Object Camera (FOC) detection. Both the magnitude and direction of the optical proper-motion components are found to be fully consistent with the most recent Very Long Baseline Array radio measurements. This result provides an unambiguous confirmation of the pulsar optical identification. In addition, we have used the combined STIS/FOC data sets to derive information on the pulsar spectrum, which seems characterized by a power-law component, apparently unrelated to the X-ray emission.

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Footnotes

  • Based on observations with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by AURA, Inc., under contract NAS5-26555.

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10.1086/345291