國立虎尾科技大學 |

Spectral Evolution in Blazars = The Case of CTA 102 /

Record Type:	Language materials, printed : Monograph/item
Title/Author:	Spectral Evolution in Blazars/ by Christian Fromm.
Reminder of title:	The Case of CTA 102 /
Author:	Fromm, Christian.
Description:	XVI, 210 p. 127 illus., 112 illus. in color.online resource. :
Contained By:	Springer Nature eBook
Subject:	Astronomy. -
Online resource:	https://doi.org/10.1007/978-3-319-10768-4
ISBN:	9783319107684

Spectral Evolution in Blazars = The Case of CTA 102 /
Fromm, Christian.

Spectral Evolution in BlazarsThe Case of CTA 102 /[electronic resource] :by Christian Fromm. - 1st ed. 2015. - XVI, 210 p. 127 illus., 112 illus. in color.online resource. - Springer Theses, Recognizing Outstanding Ph.D. Research,2190-5053. - Springer Theses, Recognizing Outstanding Ph.D. Research,.

Introduction -- Theory -- Light curve analysis -- VLBI kinematic analysis -- Core-shift and spectral analysis -- eRHD Simulations -- The jet in CTA 102. A global perspective -- Appendices.

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.

ISBN: 9783319107684

Standard No.: 10.1007/978-3-319-10768-4doiSubjects--Topical Terms:

593935
Astronomy.

LC Class. No.: QB1-991

Dewey Class. No.: 520

Spectral Evolution in Blazars = The Case of CTA 102 /
LDR:02603nam a22004215i 4500 001 963857
003 DE-He213
005 20200630160603.0
007 cr nn 008mamaa
008 201211s2015 gw | s |||| 0|eng d
020 $a 9783319107684 $9 978-3-319-10768-4
024 7 $a 10.1007/978-3-319-10768-4 $2 doi
035 $a 978-3-319-10768-4
050 4 $a QB1-991
050 4 $a QB460-466
072 7 $a PG $2 bicssc
072 7 $a SCI004000 $2 bisacsh
072 7 $a PGC $2 thema
082 0 4 $a 520 $2 23
100 1 $a Fromm, Christian. $4 aut $4 http://id.loc.gov/vocabulary/relators/aut $3 1063000
245 1 0 $a Spectral Evolution in Blazars $h [electronic resource] : $b The Case of CTA 102 / $c by Christian Fromm.
250 $a 1st ed. 2015.
264 1 $a Cham : $b Springer International Publishing : $b Imprint: Springer, $c 2015.
300 $a XVI, 210 p. 127 illus., 112 illus. in color. $b online resource.
336 $a text $b txt $2 rdacontent
337 $a computer $b c $2 rdamedia
338 $a online resource $b cr $2 rdacarrier
347 $a text file $b PDF $2 rda
490 1 $a Springer Theses, Recognizing Outstanding Ph.D. Research, $x 2190-5053
505 0 $a Introduction -- Theory -- Light curve analysis -- VLBI kinematic analysis -- Core-shift and spectral analysis -- eRHD Simulations -- The jet in CTA 102. A global perspective -- Appendices.
520 $a 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.
650 0 $a Astronomy. $3 593935
650 0 $a Astrophysics. $3 646223
650 1 4 $a Astronomy, Astrophysics and Cosmology. $3 593936
710 2 $a SpringerLink (Online service) $3 593884
773 0 $t Springer Nature eBook
776 0 8 $i Printed edition: $z 9783319107691
776 0 8 $i Printed edition: $z 9783319107677
776 0 8 $i Printed edition: $z 9783319385365
830 0 $a Springer Theses, Recognizing Outstanding Ph.D. Research, $x 2190-5053 $3 1253569
856 4 0 $u https://doi.org/10.1007/978-3-319-10768-4
912 $a ZDB-2-PHA
912 $a ZDB-2-SXP
950 $a Physics and Astronomy (SpringerNature-11651)
950 $a Physics and Astronomy (R0) (SpringerNature-43715)