color study of blazars robert filgas supervisor: rndr. rené hudec, csc., aÚ av Čr
TRANSCRIPT
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COLOR STUDY OF BLAZARS
Robert Filgas
Supervisor: RNDr. René Hudec, CSc., AÚ AV ČR
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Goals of the thesis
• To summarize and discuss known facts about blazar spectra, luminosity in optical band and its time evolution.
• To build and analyze my own database of optical photometry of blazars.
• To interpret and discuss acquired results; conclusions, comparison with theoretical models, physics of the environment.
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Active galaxies
1943 Carl Seyfert – fundamentals of AGN class (Seyfert galaxies)
Great luminosity (1042 to 1047 erg s-1) in a very compact region => supermassive black hole (107 to 109 MS) in the center of the galaxy with accretion disk, dust torus and sometimes a jet.
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Rarities of AGN
• Strong emission linesemission lines much broader than absorption lines
broadness caused by Doppler effect, gravity, velocity, temperatures
• Variability of the luminosityvariability of such giant objects unexpected
brightness can increase 1000x on scale of days
gives us the upper limit for size of the radiating area
• Differences in spectradominates non-thermal emission due to presence of active nuclei
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Types of AGN
• Blazars– name given by Ed Spiegel, 1978– these days blazar rather a phenomenon then a category of
objects– common is a relativistic jet pointed almost at us– radiation of the jet is non-thermal, relativistically boosted and
polarized
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Physical processes in jets of AGN
• Superluminal motion
• Relativistic beaming
– increasing or decreasing of the radiation intensity from the source moving with relativistic speed
where
for homogenous sphere P = 3 + α
Lorentz factor ~ 10 => boosting 100x – 1000x
!can explain why we see only one jet!
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Spectra of blazars
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Spectra of blazars
• Synchrotron emission– radiation of relativistic electron accelerated in a magnetic
field
gyrofrequency Larmor radius
energy radiated by the electron increases as
– spectrum broad and centered on the critical frequency
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Spectra of blazars
• Synchrotron emission– nature of spectrum depends on the speed of electrons
– electron energy distribution has a power-law nature =>
power-law synchrotron spectrum
– some of radio sources so compact => under certain frequency electrons optically thick for their own radiation
» synchrotron self-absorption
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Spectra of blazars
• Synchrotron emission
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Variability of blazars
• Long-term variation– variations on time scales of months to years– many models: binary BH, precession of the jet,
perturbations to the disk,..– periodicity found
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Variability of blazars• Short-term variation
– days to months– orbital motion of jet from less massive BH?
• Intraday variation– night to night variations– can give upper limit to the mass of central BH and the size
of emitting region
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Variability of blazars
• Microvariation– minutes to hours
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Causes of the variability
• Extrinsic causes
– microlensing
– interstellar scintillation
• Intrinsic causes
– accretion disk models
– geometrical effects
– shocks in jet
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Causes of the variability
• Interstellar scintillation
– result of wavefronts from a distant radio source being perturbed by refractive index fluctuations in the turbulent, ionized interstellar medium of our Galaxy
– observed only in the most compact radio sources
– principal cause of the rapid radio IDV in BL Lac objects
– !affects only radio band of the spectrum!
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Causes of the variability
• Microlensing
– one of Einstein’s general relativity predictions
– light from distant source bent around massive object
– microlensing: no distortion in shape
amount of light received increases
– brightness variations:» Symmetric outburst» Frequency independence across spectrum» Duration related to the lens speed
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Causes of the variability
• Accretion disk models
– bright spots on disks» modulation of variability by radiating flare
– vortices forming within a disk
– plasma dominated events just above disk
– spiral shocks produced in disk by passing massive stars, molecular clouds or companion BH
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Causes of the variability
• Geometrical effects• based on changing of Doppler factor
– binary BH» precession of system» gravitational lensing from the secondary BH
– helical jet models» knots or blobs of plasma spiraling in the jet
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Causes of the variability
• Shock-in-jet model– major increase in bulk velocity or internal energy of the jet
flow will cause shock waves to form and propagate down the jet
» decelerates supersonic flows to subsonic speeds
– compression of plasma and enhancement of parallel component of magnetic field
– flares results from increased density behind the shock front and increased magnetic field
– frequency dependent effect
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Causes of the variability• Shock-in-jet model
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Data analysis• Dataset
– 33 blazars – 11 LBLs, 19 HBLs and 2 FSRQs
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Data analysis• Finding power-law spectra
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Data analysis• Bluer-when-brighter tendency
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Data analysis
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Data analysis
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Data analysis• not corresponding, SED deformation (thermal contribution from host
galaxy or non-thermal contribution from different regions ?)
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Data analysis
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Data analysis• Inconsistent models:
– Interstellar scintillation – affects radio and only
– Gravitational lenses – frequency independent
• Acceptable models:
– Accretion disk models – thermal contribution from disk during quiescent state of HBLs and FSRQs
– Geometrical effects – extreme dependency on slight changes of Doppler factor, binary holes commonly accepted
– Shock-in-jet model – consistent with spectral hardening, need for data in all spectral bands
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Data analysis• Color analysis
– color-color diagrams project dispersion of light on its way to the Earth
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Data analysis
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Data analysis
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Data analysis• Color analysis
– color-color diagrams project dispersion of light on its way to the Earth
– compared with OA of GRBs we see similarities
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Data analysis
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Data analysis
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Data analysis• Color analysis
– color-color diagrams project dispersion of light on its way to the Earth
– compared with OA of GRBs we see similarities
– comparison with AGN shows large differences
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Data analysis
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Data analysis
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Data analysis• Color analysis
– color-color diagrams project dispersion of light on its way to the Earth
– compared with OA of GRBs we see similarities
– comparison with AGN shows large differences
– GRB and blazars have either similar or no environment
» possibility that dust and other environment is destructed along the line of sight by high-energy photons
» for blazars the origin for destruction might be in the jet
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Data analysis• Color-color diagram positions
– possibility to distinguish between various types of objects like it is with stars
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Data analysis
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Data analysis
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Data analysis• Conclusions
– synchrotron emission confirmed due to power-law spectra
– spectral index ~1.5 for LBLs well corresponding with theory
– bluer-when-brighter tendency observed – models
– small scatter in color-color diagrams – dust destruction
– mean values:
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THE END