Studying the spectum of PSR B0656+14

Details Studying the spectum of PSR B0656+14 Studying the spectum of PSR B0656+14

Jul 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005hst..prop10600k&link_type=abstract

HST Proposal ID #10600

Physics

Hst Proposal Id #10600 Hot Stars

Scientific paper

PSR B0656+14 is the brightest intermediate-age pulsar which has been extensively studied in X-rays and optical with different instruments. The wide-band photometry of PSR B0656+14 strongly suggests the presence of spectral features between 4000 and 11, 000 A. The sensitivity and resolution of ACS/WFC opens an opportunity to study the pulsar spectrum with a higher resolution and a better S/N than it was previously possible. This will allow us to accurately measure the pulsar spectrum, confirm the spectral features and investigate their shape and strength.

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