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pro vyhledávání: '"Leung, G. C. K."'
Autor:
Tam, P. H. T., Li, K. L., Kong, A. K. H., Takata, J., Leung, G. C. K., Cheng, K. S., Hui, C. Y.
Millisecond pulsars (MSPs) are thought to born in low-mass X-ray binaries when the neutron star has gained enough angular momentum from the accreting materials of its companion star. It is generally believed that a radio MSP is born when the neutron
Externí odkaz:
http://arxiv.org/abs/1412.4985
We report on X-ray and gamma-ray observations of the millisecond pulsar B1937+21 taken with the Chandra X-ray Observatory, XMM-Newton, and the Fermi Large Area Telescope. The pulsar X-ray emission shows a purely non-thermal spectrum with a hard photo
Externí odkaz:
http://arxiv.org/abs/1405.2148
Autor:
Takata, J., Li, K. L., Leung, G. C. K., Kong, A. K. H., Tam, P. H. T., Hui, C. Y., Wu, E. M. H., Xing, Y., Cao, Y., Tang, S., Wang, Z., Cheng, K. S.
Recent observations strongly suggest that the millisecond pulsar binary PSR J1023+0038 has developed an accretion disk since 2013 June. We present a multi-wavelength analysis of PSR J1023+0038, which reveals that 1) its gamma-rays suddenly brightened
Externí odkaz:
http://arxiv.org/abs/1312.0605
Akademický článek
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Publikováno v:
Astrophysical Journal; Jun2014, Vol. 787 Issue 2, p1-1, 1p
