Kwok, P. W., Cheng, K. S., Lau, M. M. (1991) A model of unpulsed very high energy gamma rays from the Crab Nebula and pulsar. The Astrophysical Journal, 379. 653pp. doi:10.1086/170538

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Reference Type	Journal (article/letter/editorial)
Title	A model of unpulsed very high energy gamma rays from the Crab Nebula and pulsar
Journal	The Astrophysical Journal
Authors	Kwok, P. W.		Author
	Cheng, K. S.		Author
	Lau, M. M.		Author
Year	1991 (October)	Volume	379
Publisher	IOP Publishing
DOI	doi:10.1086/170538Search in ResearchGate
	Generate Citation Formats
Mindat Ref. ID	3330133	Long-form Identifier	mindat:1:5:3330133:6
GUID	0
Full Reference	Kwok, P. W., Cheng, K. S., Lau, M. M. (1991) A model of unpulsed very high energy gamma rays from the Crab Nebula and pulsar. The Astrophysical Journal, 379. 653pp. doi:10.1086/170538
Plain Text	Kwok, P. W., Cheng, K. S., Lau, M. M. (1991) A model of unpulsed very high energy gamma rays from the Crab Nebula and pulsar. The Astrophysical Journal, 379. 653pp. doi:10.1086/170538
In	(1991) The Astrophysical Journal Vol. 379. IOP Publishing

	*Cheung, W. M., Cheng, K. S. (1993) A model of unpulsed gamma rays from the Crab pulsar. The Astrophysical Journal, 413. 694pp. doi:10.1086/173037*
	*Cheung, W. M., Cheng, K. S. (1994) Unpulsed high-energy radiation from the Crab pulsar and nebula. The Astrophysical Journal Supplement Series, 90. 827 doi:10.1086/191910*
	Cheng, K S, Cheung, T, Lau, M M, Yu, K N, Kwok, P W (1990) Could very high energy gamma rays from the Crab Nebula result from p-p collision?. Journal of Physics G: Nuclear and Particle Physics, 16 (7). 1115-1121 doi:10.1088/0954-3899/16/7/022
	*Cheng, K. S., Yu, K. N., Cheung, T., Lau, M. M. (1991) Very high energy gamma-ray emission from accreting X-ray pulsars. The Astrophysical Journal, 379. 290pp. doi:10.1086/170504*
	*McBreen, B., Ball, S. E., Jr., Campbell, M., Greisen, K., Koch, D. (1973) Pulsed high-energy gamma rays from the Crab Nebula. The Astrophysical Journal, 184. 571pp. doi:10.1086/152350*
	*Grindlay, J. E. (1972) Detection of Pulsed Gamma Rays of ~10^{12} EV from the Pulsar in the Crab Nebula. The Astrophysical Journal, 174. doi:10.1086/180939*
	*Golden, A., Shearer, A., Beskin, G. M. (2000) Unpulsed Optical Emission from the Crab Pulsar. The Astrophysical Journal, 535 (1). 373-378 doi:10.1086/308826*
	*Fazio, G. G., Helmken, H. F., O'Mongain, E., Weekes, T. C. (1972) Detection of High-Energy Gamma Rays from the Crab Nebula. The Astrophysical Journal, 175. doi:10.1086/180998*
	*Wei, D. M., Cheng, K. S., Lu, T. (1996) Pulsed and Unpulsed Gamma-Ray Emission from Millisecond Pulsars. The Astrophysical Journal, 468. 207pp. doi:10.1086/177683*
	Vacanti, G., Cawley, M. F., Colombo, E., Fegan, D. J., Hillas, A. M., Kwok, P. W., Lang, M. J., Lamb, R. C., Lewis, D. A., Macomb, D. J., O'Flaherty, K. S., Reynolds, P. T., Weekes, T. C. (1991) Gamma-ray observations of the Crab Nebula at TeV energies. The Astrophysical Journal, 377. 467pp. doi:10.1086/170376
	*Takata, J., Chang, H.‐K., Cheng, K. S. (2007) Polarization of High‐Energy Emission from the Crab Pulsar. The Astrophysical Journal, 656 (2). 1044-1055 doi:10.1086/510190*

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Kwok, P. W., Cheng, K. S., Lau, M. M. (1991) A model of unpulsed very high energy gamma rays from the Crab Nebula and pulsar. The Astrophysical Journal, 379. 653pp. doi:10.1086/170538

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