Chandra Detailed Spatial Study of the ``ANOMALOUS'' - Pulsars

Details Chandra Detailed Spatial Study of the ``ANOMALOUS'' - Pulsars Chandra Detailed Spatial Study of the ``ANOMALOUS'' - Pulsars

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000cxo..prop..607i&link_type=abstract

Chandra Proposal ID #02500518

Physics

Chandra Proposal Id #02500518

Scientific paper

We propose here to observe the sample of AXPs with the Chandra HRC-I in order to improve their X-ray positions (down to 1'' or better). This level of positional accuracy is indispensable to identify the optical/IR counterparts of AXPs in their crowded galactic plane fields. We plan to use the X-ray emission of known bright K-M spectral type stars within the field of view (FOV) of HRC-I which are nearby (within a radius of about 15') each AXP. We also will investigate the presence of extended emission around AXPs: in particular 2E2259+58, AXJ1844-0258 and 1E1841-04 are likely associated with known shell-like radio emission which will be studied in detail.

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