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MODULATION INDEX – GALACTIC LATITUDE RELATION G. Tsarevsky ASTRO SPACE CENTER, Moscow
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EXTRAGALACTIC SOURCES RADIO VARIABILITY
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INTRINSIC?
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EXTRAGALACTIC SOURCES RADIO VARIABILITY INTRINSIC? EXTRINSIC?
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QSO is an essentially variable stuff!
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It should vary in radio as well !
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It should vary in radio as well, and it really vary!
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Blazar 1514+197 Green Bank Interferometer data Intrinsic variation is over month to year, stronger at 8 GHz. ISS is the variation over day to week, stronger at 2 GHz
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H. D. Aller, M. F. Aller, Ph. A. Hughes, G. E. Latimer: University of Michigan Radio Observatory (UMRAO) Database 26-m dish; 4.8, 8.0, 14.5 GHz (including polarisation!), 25 years http://www.astro.lsa.umich.edu/obs/radiotel/umrao.html E. B. Waltman et al., ApJS 77, 379, 1991: Green Bank Interferometer (GBI) Daily Observations Database 2.25 and 8.3 GHz, 17 years http://www.gb.nrao.edu/fgdocs/gbi/gbint.html http://www.astro.lsa.umich.edu/obs/radiotel/umrao.html
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ISS Geometry From Radio Galaxy Quasar or AGN 2000 pc
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Center Anticenter Poles: Center Anticenter Poles: ↓ C > AC > Poles
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What about m - |b| plot behavior?
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ApJ 618,108-140, 2004 Radio Variability of Radio Quiet and Radio Loud Quasars Richard Barvainis Joseph Leh´ar Mark Birkinshaw Heino Falke Katherine M. Blundell
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ApJ 618,108-140, 2004 Radio Variability of Radio Quiet and Radio Loud Quasars Richard Barvainis Joseph Leh´ar Mark Birkinshaw Heino Falke Katherine M. Blundell Subject headings: Quasars; Active Galaxies; Radio Emission
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VLA monitoring of RLQ and RQQ
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Some refs: N. Shapirovskaya, O.B. Slee, P. Hughes, & G. Tsarevsky "Radio Source Variability as a Tool for Very High Resolution" In: Proc. IAU Symposium No. 158, Sydney, eds. J. Robertson & W. Tango, Kluwer Acad. Press, 1993, p. 201-203 N. Shapirovskaya, O.B. Slee, & G. Tsarevsky "Galaxy Centre-Anticentre Asymmetry of the LFV Radio Source Distribution : Evidence of the Interstellar Matter Influence" In: Sub-arcsecond Radio Astronomy, eds. R. Davies & R. Booth, CUP, 1993, p.94 - 95
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