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000746060 019__ $$a908090113
000746060 020__ $$a9783319107684$$qelectronic book
000746060 020__ $$a3319107682$$qelectronic book
000746060 020__ $$z9783319107677
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000746060 0247_ $$a10.1007/978-3-319-10768-4$$2doi
000746060 035__ $$aSP(OCoLC)ocn890319261
000746060 035__ $$aSP(OCoLC)890319261$$z(OCoLC)908090113
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000746060 049__ $$aISEA
000746060 050_4 $$aQB858.35
000746060 08204 $$a523.11$$223
000746060 1001_ $$aFromm, Christian,$$eauthor.
000746060 24510 $$aSpectral evolution in blazars$$h[electronic resource] :$$bthe case of CTA 102 /$$cChristian Fromm.
000746060 264_1 $$aCham :$$bSpringer,$$c[2015]
000746060 264_4 $$c©2015
000746060 300__ $$a1 online resource.
000746060 336__ $$atext$$btxt$$2rdacontent
000746060 337__ $$acomputer$$bc$$2rdamedia
000746060 338__ $$aonline resource$$bcr$$2rdacarrier
000746060 4901_ $$aSpringer theses
000746060 500__ $$a"Doctoral thesis accepted by the Rheinischen Friedrich-Wilhelms-Universität Bonn, Germany."
000746060 504__ $$aIncludes bibliographical references.
000746060 5050_ $$aIntroduction -- Theory -- Light curve analysis -- VLBI kinematic analysis -- Core-shift and spectral analysis -- eRHD Simulations -- The jet in CTA 102. A global perspective -- Appendices.
000746060 506__ $$aAccess limited to authorized users.
000746060 520__ $$aThis prize-winning thesis deals with the observation and modeling of the spectral evolution of blazars. Based on single-dish light curves, a model of shock-shock interaction is tested and confirmed using multi-frequency high resolution Very Long Baseline Observations. He presents state-of-the art numerical relativistic hydrodynamic simulations and the corresponding non-thermal emission is calculated (eRHD simulations). The author further presents new analysis techniques for VLBI observations that can be applied to numerous sources and provide reliable results including an error estimate using Monte Carlo simulations. He also develops an analytical shock model that can be applied quickly to other single dish observations. He shows how novel techniques of extraction of physical parameters from observations can be applied to other astrophysical sources and provide a link to a better understanding of the physical mechanism operating in blazar jets.
000746060 588__ $$aDescription based on print version record.
000746060 650_0 $$aBL Lacertae objects.
000746060 650_0 $$aAstrophysical jets.
000746060 650_0 $$aActive galaxies.
000746060 650_0 $$aAstrophysics.
000746060 77608 $$iPrint version:$$tSpectral Evolution in Blazars$$z9783319107677$$w(OCoLC)886485700
000746060 830_0 $$aSpringer theses.
000746060 85280 $$bebk$$hSpringerLink
000746060 85640 $$3SpringerLink$$uhttps://univsouthin.idm.oclc.org/login?url=http://link.springer.com/10.1007/978-3-319-10768-4$$zOnline Access$$91397441.1
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000746060 980__ $$aEBOOK
000746060 980__ $$aBIB
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