BID 发表于 2025-3-21 20:01:59

书目名称Extragalactic Radio Sources影响因子(影响力)<br>        http://figure.impactfactor.cn/if/?ISSN=BK0319977<br><br>        <br><br>书目名称Extragalactic Radio Sources影响因子(影响力)学科排名<br>        http://figure.impactfactor.cn/ifr/?ISSN=BK0319977<br><br>        <br><br>书目名称Extragalactic Radio Sources网络公开度<br>        http://figure.impactfactor.cn/at/?ISSN=BK0319977<br><br>        <br><br>书目名称Extragalactic Radio Sources网络公开度学科排名<br>        http://figure.impactfactor.cn/atr/?ISSN=BK0319977<br><br>        <br><br>书目名称Extragalactic Radio Sources被引频次<br>        http://figure.impactfactor.cn/tc/?ISSN=BK0319977<br><br>        <br><br>书目名称Extragalactic Radio Sources被引频次学科排名<br>        http://figure.impactfactor.cn/tcr/?ISSN=BK0319977<br><br>        <br><br>书目名称Extragalactic Radio Sources年度引用<br>        http://figure.impactfactor.cn/ii/?ISSN=BK0319977<br><br>        <br><br>书目名称Extragalactic Radio Sources年度引用学科排名<br>        http://figure.impactfactor.cn/iir/?ISSN=BK0319977<br><br>        <br><br>书目名称Extragalactic Radio Sources读者反馈<br>        http://figure.impactfactor.cn/5y/?ISSN=BK0319977<br><br>        <br><br>书目名称Extragalactic Radio Sources读者反馈学科排名<br>        http://figure.impactfactor.cn/5yr/?ISSN=BK0319977<br><br>        <br><br>

effrontery 发表于 2025-3-21 22:54:44

https://doi.org/10.1007/978-3-8349-8522-4 observations of Cygnus A at 22 & 43 GHz, which reveal evidence for subluminal motion in jet and counter-jet, and 86 GHz VLBI observations of two extreme γ—blazars, suggesting a tight correlation between their γ—ray activity and the generation of jets.

nuclear-tests 发表于 2025-3-22 01:53:43

Das digitalisierte Kontrollorgan?1 in comparison to the status of 0528+134 in the EGRET energy range. The uncertainties in the flux densities quoted there are less than 5% at 10.55 GHz and lower frequencies, while slightly exceeding this value at 32 GHz and 86 GHz.

Pandemic 发表于 2025-3-22 07:09:22

https://doi.org/10.1007/978-3-322-84818-5 found a single component with . = 8 × 10. K. One year later, within one week of the peak of flare at 3 mm λ, observations with Haystack, Kitt Peak and Hat Creek observatories revealed a component comparable in size and flux density with . = 7 × 10. K. Table 1 details the source models for the two experiments.

多骨 发表于 2025-3-22 12:09:48

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AORTA 发表于 2025-3-22 13:08:58

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AORTA 发表于 2025-3-22 20:13:36

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ear-canal 发表于 2025-3-22 23:46:24

Conference proceedings 1996ve days, to update their knowledge of thephysics and statistical properties of powerful extragalactic radiosources. .Since their discovery in the fifties enormous progress has been made.The existence of superluminal motions in the cores of radio sources,the presence there of a black hole surrounded

教唆 发表于 2025-3-23 03:56:18

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是比赛 发表于 2025-3-23 06:42:39

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查看完整版本: Titlebook: Extragalactic Radio Sources; Proceedings of the 1 R. Ekers,C. Fanti,L. Padrielli Conference proceedings 1996 International Astronomical Uni