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Publisher: Elsevier

Volume 22, Number 2, 1998

Superluminal source candidates 0208-512 and 2243-123
pp. 133-137(5)
Authors: Shen, Z.-Q.; Hong, X.-Y.; Wan, T.-S.

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Is the jet of AO 0235+164 rotating?
pp. 138-144(7)
Authors: Zhang, F.-J.; Chen, Y.-J.; Zhu, H.-S.

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Stellar population synthesis for the spectra of blue compact galaxies
pp. 145-154(10)
Authors: Xu, K.; Cheng, F.-Z.

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Correlation between TeV and X-ray bursts in Mrk 421
pp. 155-160(6)
Authors: Qian, S.-J.; Zhang, X.-Z.; Witzel, A.; Krichbaum, T.; Britzen, S.; Kraus, A.

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Convective instability in the prompt explosion model of Type-II supernovae
pp. 161-165(5)
Authors: Zhang, S.-C.; Xie, Z.-H.; Wang, Y.-R.; Wang, W.-Z.

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Geminga: why it is not a radio pulsar
pp. 166-174(9)
Authors: Wang, Z.-X.; Tan, L. U.

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A study of phase relations in gamma-ray pulsars
pp. 175-178(4)
Authors: Wang, Z.-X.; Tan, L. U.

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Unusual phenomena in the new emission phase of X Persei
pp. 192-197(6)
Authors: Liu, Q.-Z.; Hang, H.-R.

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A self-modulation model of solar radio emission
pp. 198-204(7)
Authors: Wang, D.-.; Huang, G.-L.; Mao, D.-Y.

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Excitation of solar p-modes
pp. 205-214(10)
Authors: Bi, S.-I.; Li, R.-F.

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Observation of an explosion in Comet Hale-Bopp
pp. 215-217(3)
Authors: Qian, B.-C.; Gu, M.-F.; Tao, J.; Pan, H.-J.

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A method of analyzing incomplete times series with application to two cataclysmic variables
pp. 235-242(8)
Authors: Ding, Y.-R.; Zhao, H.-H.; Li, Z.-Y.

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