نتایج جستجو برای: 096
تعداد نتایج: 469 فیلتر نتایج به سال:
Different properties of quasars may be observed and analysed through the many ranges electromagnetic spectrum. Pioneering studies showed that an "H-R diagram" for was needed to organize these data, more than two dimensions were necessary: a four dimensional Eigenvector (4DE1) parameter space proposed. The 4DE1 makes use independent observational obtained from optical UV emission lines, as well ...
Pressure dependence of infrared absorption has been measured in Cs2TCNQ3 single crystals grown under magnetic field of 5 T (5 T crystals). The behavior of the C-CN as well as C-H stretching modes suggest that there occurs a phase transition which resembles to the one related to the insulator to metal transition in the crystals grown without magnetic field (0 T crystals). This transition, howeve...
Based on the two epochs EVN archive data from OH line observations of IIZw 096, we confirm that high-resolution emission in this source mainly comes spots (OH1 and OH2) comp D1 merging system. We found no significant variations emission. The 1665 MHz is detected at about 6 $\sigma$ level OH1 region by combining epoch observations. shows brightest CO, HCO+ emission, as well multi-band radio cont...
We present results and first epoch parsec-scale images from a monitoring program on five γ–ray loud blazars selected on the basis of their total flux density variability. We observed 0048−097, 0235+164, 0954+658, 1510−089 and 1749+096 with the Very Long Baseline Array simultaneously at 8.4 GHz and 22 GHz. Comparison between our high quality images and previous results from the literature sugges...
[*] Prof. Z. L. Wang, Y.-F. Lin, J. H. Song, Dr. Y. Ding School of Materials Science and Engineering Georgia Institute of Technology Atlanta, GA 30332-0245 (USA) E-mail: [email protected] Prof. S.-Y. Lu, Y.-F. Lin Department of Chemical Engineering National Tsing Hua University Hsin-Chu, Taiwan 30013 (ROC) E-mail: [email protected] [**] This work was supported by the DOE BES (DE-FG02-...
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