-28%
80,95
Bisher 111,99**
80,95
Alle Preise in Euro, inkl. MwSt.
**Preis der gedruckten Ausgabe (Gebundenes Buch)
Sofort per Download lieferbar
Bisher 111,99**
80,95
Alle Preise in Euro, inkl. MwSt.
**Preis der gedruckten Ausgabe (Gebundenes Buch)
Sofort per Download lieferbar

Alle Infos zum eBook verschenken
Als Download kaufen
Bisher 111,99**
-28%
80,95
Preis in Euro, inkl. MwSt.
**Preis der gedruckten Ausgabe (Gebundenes Buch)
Sofort per Download lieferbar
Abo Download
9,90 / Monat*
*Abopreis beinhaltet vier eBooks, die aus der tolino select Titelauswahl im Abo geladen werden können.

Preis in Euro, inkl. MwSt.
Sofort per Download lieferbar

Einmalig pro Kunde einen Monat kostenlos testen (danach 9,90 pro Monat), jeden Monat 4 aus 40 Titeln wählen, monatlich kündbar.

Mehr zum tolino select eBook-Abo
Jetzt verschenken
Bisher 111,99**
-28%
80,95
Preis in Euro, inkl. MwSt.
**Preis der gedruckten Ausgabe (Gebundenes Buch)
Sofort per Download lieferbar

Alle Infos zum eBook verschenken
40 °P sammeln

  • Format: PDF


This 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
…mehr

  • Geräte: PC
  • ohne Kopierschutz
  • eBook Hilfe
  • Größe: 15.14MB
Produktbeschreibung
This 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.

Dieser Download kann aus rechtlichen Gründen nur mit Rechnungsadresse in A, B, BG, CY, CZ, D, DK, EW, E, FIN, F, GB, GR, HR, H, IRL, I, LT, L, LR, M, NL, PL, P, R, S, SLO, SK ausgeliefert werden.

Autorenporträt
Christian Fromm received his PhD in Astronomy and Astrophysics from University of Bonn/ MPIfR, Germany, in December 2012. It was nominated for publication as Springer Thesis by MPIfR. He is now working as postdoctoral researcher at the German Aerospace Centre, Institut for Space Propulsion.
Inhaltsangabe
Introduction.- Theory.- Light curve analysis.- VLBI kinematic analysis.- Core-shift and spectral analysis.- eRHD Simulations.- The jet in CTA 102. A global perspective.- Appendices.