Optical and IR imaging of the locality of 1E2259 + 586

Details Optical and IR imaging of the locality of 1E2259 + 586 Optical and IR imaging of the locality of 1E2259 + 586

Mar 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991mnras.249..313d&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 249, March 15, 1991, p. 313-318.

Astronomy and Astrophysics

Astronomy

19

Infrared Imagery, Pulsars, Supernova Remnants, X Ray Binaries, Accretion Disks, Astrometry, Astronomical Photometry, Blue Stars, Visible Spectrum

Scientific paper

New optical and IR images of the locality of the X-ray pulsar 1E2259 + 586, as well as revised astrometry are presented. Although the optical counterpart cannot be conclusively identified, several new candidates are identified, including one which is particularly blue. The implications of the results are discussed for LMXRB models of 1E2259 + 586: one possibility is that the pulsar is not physically related to the surrounding SNR G109.1 - 1.0.

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