Unveiling the X-ray properties of the new Geminga-like pulsar: PSR J2021+4026

Details Unveiling the X-ray properties of the new Geminga-like pulsar: PSR J2021+4026 Unveiling the X-ray properties of the new Geminga-like pulsar: PSR J2021+4026

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010xmm..prop...20h&link_type=abstract

XMM-Newton Proposal ID #06705901

Computer Science

Supernovae, Supernova Remnants, Diffuse (Galactic) Emission And Isolated Neutron Stars, Psr J2021+4026

Scientific paper

PSR J2021+4026 is the second brightest radio-quiet gamma-ray pulsar which is suggested to be the long-sought compact object associated with the supernova remnant gamma-Cygni. Its radio-quietness and its multiwavelength properties suggest its nature to be similar to a well-known pulsar: Geminga. In order to tightly constrain the nature of its X-ray counterpart, we propose a deep XMM-Newton observation with an aim to search for its X-ray pulsations and perform a detailed spectro-imaging analysis.

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