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活动星系核的射电精细结构和光变观测研究     活动星系核  射电精细结构  光变观测       font style='font-size:12px;'> 2023/8/12
活动星系核的射电精细结构和光变观测研究
The Balmer H alpha emission line in the stationary spectrum of SS 433 has a component originating in the wind above the accretion disk. The Doppler motion of this line is a blurred representation of t...
We report on the high precision timing analysis of the pulsar-white dwarf binary PSR J1012+5307. Using 15 years of multi-telescope data from the European Pulsar Timing Array (EPTA) network, a signific...
Large scale absorbers in the environment of high-z radio-galaxies     high-z  radio-galaxies       font style='font-size:12px;'> 2009/6/30
Large scale absorbers in the environment of high-z radio-galaxies。
VLA Detection of a Double Radio Source at the Center of the HH 288 Quadrupolar Outflow。
Tomography of high redshift clusters with OSIRIS     high redshift  Tomography       font style='font-size:12px;'> 2009/6/12
Tomography of high redshift clusters with OSIRIS。
VLA Detection of the Exciting Sources of the Molecular Outflows Associated with L1448 IRS2, IRAS 05327+3404, L43, IRAS 22142+5206, L1211, and IRAS 23545+6508。
Ray-tracing calculations show that a trough, L = 4.6, located in the region outside the plasmapause is capable to guide whistler-mode waves in frequency range 0.5fBmin−0.64fBmin, from one hemi...

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