270 likes | 420 Vues
Yu.N.Vetukhnovskay, V.E. Yakimov , D.Gabuzda. Jets polarization and spectral properties of 18 gamma-ray quasars. Observations: VLBA ,frequencies 5 and 15 GHz, two circular polarizations. Calibration: AIPS usual tasks.
E N D
Yu.N.Vetukhnovskay, V.E. Yakimov , D.Gabuzda Jets polarization and spectral properties of 18 gamma-ray quasars
Observations: VLBA ,frequencies 5 and 15 GHz, two circular polarizations. Calibration: AIPS usual tasks. Images: AIPS, DIFMAP . Model fitting: DIFMAT, VISFIT
0202+149 0.405 0.827+247 0.941 1611+343 1.401 0234+285 1.207 1156+295 0.729 1633+382 1.807 0420-014 0.915 1222+216 0.435 1739+522 1.381 0446+112 1.207 1406-076 1.494 1741-038 1.054 0528+134 2.070 1510-089 0.360 2022-077 1.388 0804+499 1.432 1606+106 1.226 2230+114 1.037 name z name z name z
1741-038 is optically thick (Kovalev et al, 1999) The core and jet of 0202+149 is unpolarized at 15 GHz (<0.5%) At 15 GHz jet of 2022-077 is also unpolarized (<0.3%)
The jets of of gamma-ray-quasars may be extent (1606+106 and 2230+114) The length of jet of 1611+343 is the same from 5 to 43 Ghz Spine-sheath polarization structure of 1606+106
The fractional polarization of the components for models of quasarsmaybe >30%. Components I and P not always coincide. In greycolour for 1611+343 and 1633+382 the fractional polarizationdistribution at two frequencies.
Definition of the Rotation Measure for two frequencies is not correct, but it is sometimes interesting. Example - RM for 1633+382
TheAIPStaskCOMBwasusedforspectralindexdefinition. Thecorepositionfor 5 and15GHZ are different (Lobanov,1998 andreferencestherein; Pushkarevetal, 2008) Mapsattwofrequencieswiththesamebeamwidth. Modelfittingandopticallythincomponentsattwomaps.
The core shifts 0202+149 0.82 mas 1606+106 0.37 mas 0234+285 0.43 mas 1611+343 0.40 mas 0827+243 0.00 mas 1633+382 0.73 mas 1222+216 0.64 mas 2230+114 0.94 mas 1406-076 0.13 mas