Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/6906
Title: Phase-resolved X-ray polarimetry of the Crab pulsar with the AstroSat CZT Imager.
Authors: Vadawale, S.V.
Chattopadhyay, T.
Paul, Biswajit
+14 Co-authors
Issue Date: Jan-2018
Publisher: Macmillan Publishers
Citation: Nature Astronomy, 2018, Vol. 2, p50-55
Abstract: The Crab pulsar is a typical example of a young, rapidly spinning, strongly magnetized neutron star that generates broadband electromagnetic radiation by accelerating charged particles to near light speeds in its magnetosphere1. Details of this emission process so far remain poorly understood. Measurement of polarization in X-rays, particularly as a function of pulse phase, is thought to be a key element necessary to unravel the mystery of pulsar radiation2,3,4. Such measurements are extremely difficult, however: to date, Crab is the only pulsar to have been detected in polarized X-rays5,6,7,8 and the measurements have not been sensitive enough to adequately reveal the variation of polarization characteristics across the pulse7. Here, we present the most sensitive measurement to date of polarized hard X-ray emission from the Crab pulsar and nebula in the 100–380 keV band, using the Cadmium–Zinc–Telluride Imager9 instrument on-board the Indian astronomy satellite AstroSat10. We confirm with high significance the earlier indication6,7 of a strongly polarized off-pulse emission. However, we also find a variation in polarization properties within the off-pulse region. In addition, our data hint at a swing of the polarization angle across the pulse peaks. This behaviour cannot be fully explained by the existing theoretical models of high-energy emission from pulsars.
Description: Restricted Access.
URI: http://hdl.handle.net/2289/6906
ISSN: 2397-3366 (online)
Alternative Location: http://adsabs.harvard.edu/abs/2018NatAs...2...50V
http://dx.doi.org/10.1038/s41550-017-0293-z
Copyright: 2018 Macmillan Publishers
Appears in Collections:Research Papers (A&A)

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