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

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書目名稱Extragalactic Radio Sources影響因子(影響力)




書目名稱Extragalactic Radio Sources影響因子(影響力)學(xué)科排名




書目名稱Extragalactic Radio Sources網(wǎng)絡(luò)公開度




書目名稱Extragalactic Radio Sources網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Extragalactic Radio Sources被引頻次




書目名稱Extragalactic Radio Sources被引頻次學(xué)科排名




書目名稱Extragalactic Radio Sources年度引用




書目名稱Extragalactic Radio Sources年度引用學(xué)科排名




書目名稱Extragalactic Radio Sources讀者反饋




書目名稱Extragalactic Radio Sources讀者反饋學(xué)科排名

effrontery

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

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

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.

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AORTA

AORTA

ear-canal

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

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