Ejaculate
发表于 2025-3-23 12:19:30
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Perineum
发表于 2025-3-23 14:53:01
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Meditate
发表于 2025-3-23 20:00:35
The Sub-Parsec Scale Jets of AGN 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.
HUMID
发表于 2025-3-24 01:03:03
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Bureaucracy
发表于 2025-3-24 03:28:05
A Dramatic (and Invisible!) Flare in NRAO 530 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.
Suppository
发表于 2025-3-24 09:06:39
High Frequency Radio Observations of the Nucleus of Cen Arays (Kinzer et al. 1995). In the radio domain, the emission from the core dominates at high frequencies and a considerable effort was made to study variability at 22 and 43 GHz for more than ten years (Botti & Abraham 1995).
Macronutrients
发表于 2025-3-24 13:23:43
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Inferior
发表于 2025-3-24 16:13:58
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florid
发表于 2025-3-24 20:00:08
Betriebs- und Wirtschaftsinformatikfar side jets are similar. This was interpreted as the result of free-free absorption in an ionized medium that lies in front of the counterjet but not in front of the near-side jet. An accretion disk or torus has an appropriate geometry to show this effect (for an analysis, see Levinson .., 1995).
CROW
发表于 2025-3-25 02:39:07
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