搜索结果: 1-8 共查到“知识库 射电天文方法”相关记录8条 . 查询时间(1.589 秒)
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
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2023/8/12
活动星系核的射电精细结构和光变观测研究
SS 433: The wiggle of the wind
stars: individual: SS 433 - binaries: close - stars: fundamental parameters - winds
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2011/10/13
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...
Precision timing of PSR J1012+5307 and strong-field GR tests
PSR J1012+5307 dipole radiation gravitational constant variation
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2010/3/19
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
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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
VLA HH 288 Quadrupolar Outflow Double Radio
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2009/6/16
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
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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
Molecular Outflows IRAS 05327+3404 L1448 IRS2 IRAS 22142+5206
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2009/6/11
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。
GUIDING OF WHISTLER-MODE WAVES WITH FREQUENCIES ABOVE ONE HALF OF THE GYROFREQUENCY IN THE MAGNETOSPHERE
WHISTLER-MODE WAVES GYROFREQUENCY MAGNETOSPHERE FREQUENCIES
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2009/3/19
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...