HST/NICMOS observations of PSR 0656+14 and Geminga

Details HST/NICMOS observations of PSR 0656+14 and Geminga HST/NICMOS observations of PSR 0656+14 and Geminga

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aas...193.4107h&link_type=abstract

American Astronomical Society, 193rd AAS Meeting, #41.07; Bulletin of the American Astronomical Society, Vol. 30, p.1309

Astronomy and Astrophysics

Astronomy

4

Scientific paper

We present results of March 1998 NICMOS observations of two middle-aged pulsars, PSR 0656+14 and Geminga, with three and two broad-band filters, respectively. The infrared fluxes of both objects grow with increasing wavelength. Most likely they are generated in the pulsars' magnetospheres. Composite UV/optical/IR spectral fluxes of the pulsars demonstrate that the radiation in this wavelength range cannot be described by a simple one-component model.

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