13353 BI-H-1013-001 HONORS BIOL OF THE CELL U 3 GRIPPO A MTG1-TR 0930AM-1100AM LSE 207 10990 EN-H-1013-001 HONORS FR ENGLISH II U 3 MCGHEE R MTG1-MWF 0900AM-0950AM W 315 10991 EN-H-1013-002 HONORS FR ENGLISH II U 3 SCHICHLER R MTG1-TR 1100AM-1215PM LIB 103B 10992 EN-H-1013-003 HONORS FR ENGLISH II U 3 CHAPPEL D MTG1-MWF 1200PM-1250PM LIB 103B 10993 EN-H-2013-001 HNRS INTRO LIT II U 3 COLLINS J ...

Pictor A is a nearby Fanaroff-Riley class II (FR II) radio galaxy with a bright hot spot, the western hot spot. Observation of high polarization in the optical emission of the hot spot indicates that the optical emission could be synchrotron radiation of relativistic electrons in the hot spot. These electrons may be able to produce high energy γ-ray photons through inverse Compton (IC) scatteri...

The purpose of this investigation was to compare the dentoalveolar and skeletal cephalometric changes produced by the Fränkel (FR-2) and bionator appliances in persons with Class II malocclusion. Lateral cephalograms were available for 66 patients of both sexes, who were divided into 3 groups of 22. The control group included untreated Class II children, with an initial mean age of 8 years 7 mo...

This retrospective cephalometric study compares the treatment effects produced in 40 patients treated with the Twin-block appliance to those seen in a matched sample of 40 children treated with the FR-2 appliance of Fränkel and to changes undergone in 40 untreated Class II controls from The University of Michigan Elementary and Secondary School Growth Study. The average starting ages for the Tw...

The experimental study of the seepage processes' sources formation in structures Arctic Region was carried out using modified methods frequency-resonance (FR) processing and decoding satellite images photographs with vertical scanning cross-sections. newly obtained results show that intensity dynamics methane seeps pockmarks fields’ depend on active deep degassing processes continental margin s...

We extend our study of the nuclei of 3CR FR II radio galaxies through HST optical images up to z = 0.3. In the majority of them an unresolved nucleus (central compact core, CCC) is found. We analyze their position in the plane formed by the radio and optical nuclear luminosities in relation to their optical spectral properties. The broad–lined objects (BLO) have the brightest nuclei: they are p...