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Discovery of an X-ray nebula in the field of millisecond pulsar PSRJ1911-1114

Author(s)
Lee, JongsuHui, C. Y.Takata, J.Lin, L. C. C.
Issued Date
2018-12
DOI
10.1051/0004-6361/201833760
URI
https://scholarworks.unist.ac.kr/handle/201301/25544
Fulltext
https://www.aanda.org/articles/aa/abs/2018/12/aa33760-18/aa33760-18.html
Citation
ASTRONOMY & ASTROPHYSICS, v.620, pp.L14
Abstract
We have discovered an extended X-ray feature, apparently associated with millisecond pulsar (MSP) PSR J1911-1114. The feature, which extends for similar to 1', was discovered from an XMM-Newton observation; the radio timing position of PSR J1911-1114 is in the midpoint of the feature. The orientation of the feature is similar to the proper motion direction of PSR J1911-1114. Its X-ray spectrum can be well-modeled by an absorbed power law with a photon index of Gamma = 1.8(-0.2)(+0.3). If this feature is confirmed to be a pulsar wind nebula (PWN), this will be the third case where an X-ray PWN has been found to be powered by a MSP.
Publisher
EDP SCIENCES S A
ISSN
1432-0746
Keyword (Author)
pulsars: individual: PSR J1911-1114X-rays: starsstars: neutron

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