tev-band galactic scienceveritasj.sao.arizona.edu/10years/talks/mp_galactic... · 2017. 6. 28. ·...
TRANSCRIPT
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TeV-band galactic science
Martin Pohl
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Introduction
Galactic science is rich!
• Supernova remnants
• Pulsar wind nebulae
• Pulsars
• Binaries
• The Galactic center
10 years VERITAS Jun 28-29, 2017
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The Galactic center
VERITAS is particularly sensitive to multi-TeV gamma rays
No evidence for variability
Do we really see Sgr A*?
10 years VERITAS Jun 28-29, 2017
Sgr A*
Power-law spectrum extends to 20 TeV
High statistical accuracy above 10 TeV
Precise measurement of cut off
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The Galactic center
Extended emission ( first seen with H.E.S.S.)
Sgr A* subtracted
G0.9+0.1 subtracted
Extended source VER J1746-289
Appears point-like in HESS data
Possibly associated with radio arc
Energy-dependent extent?
10 years VERITAS Jun 28-29, 2017
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Supernova remnants
In the early 2000‘s we knew for certain
• Galactic supernova remnants accelerate to PeVs
• Cosmic-ray spectra are hard in the TeV band
• We can distinguish leptonic and hadronic g rays
10 years VERITAS Jun 28-29, 2017
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Supernova remnants
In the early 2000‘s we knew for certain
• Galactic supernova remnants accelerate to PeVs
• Cosmic-ray spectra are hard in the TeV band
• We can distinguish leptonic and hadronic g rays
Now we know better …
10 years VERITAS Jun 28-29, 2017
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Supernova remnants
IC 443: The messy supernova remnant
Little, if any, spectral variation
10 years VERITAS Jun 28-29, 2017
Green – Radio Red – Optical Blue – X-rays
VERITAS 3, 6, 9 s contours
Lee at al. 2012
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Supernova remnants
10 years VERITAS Jun 28-29, 2017
Hard spectra expected in the TeV band
… not really seen, spectra tend to be soft
Cosmic-ray spectra Gamma-ray spectra
From a paper published in 2006
Energy in TeV 0.1 1 10
Expected
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Supernova remnants
10 years VERITAS Jun 28-29, 2017
Model refinements are explored.
• Motion of scattering turbulence
• Secondary acceleration by turbulence
• Imperfect build-up of turbulence
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Supernova remnants: Cas A
10 years VERITAS Jun 28-29, 2017
How to make sense of that? Chandra X rays
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Supernova remnants: Cas A
10 years VERITAS Jun 28-29, 2017
It‘s the magnetic field, stupid! Chandra X rays
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Supernova remnants: Cas A
Weaker magnetic field Stronger magnetic field
Electrons: magenta and green Hadrons: blue
Distinguishing requires information at 1-400 MeV
10 years VERITAS Jun 28-29, 2017
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Tycho‘s Supernova remnant
Type Ia Supernova clean environment
Excess map
Statistical analysis:
Signal comes from
remnant itself
10 years VERITAS Jun 28-29, 2017
Molecular cloud
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Tycho‘s Supernova remnant
Direct, model-independent
assessment of
average magnetic field
With damping B>170 mG
10 years VERITAS Jun 28-29, 2017
2011
Data of 2017
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Pulsars
Some supernovae
leave behind a pulsar
10 years VERITAS Jun 28-29, 2017
Crab nebula and pulsar
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Crab pulsar
Gamma-ray not produced at inner acceleration gap
but rather close to or
beyond the light cylinder
2011 no absorption
10 years VERITAS Jun 28-29, 2017
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Pulsar wind nebula
MGRO J1908+06 resolved with VERITAS
A pulsar outside the remnant of its parent supernova
No evidence
of spectral variation
Complex interaction
between PWN and SNR?
Black contours: CO
10 years VERITAS Jun 28-29, 2017
Map of excess counts
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Pulsar wind nebula
Spectral variability is normal in composite sources
Example: MGRO J2019+37 resolved with VERITAS
10 years VERITAS Jun 28-29, 2017
Map of excess counts > 1 TeV < 1 TeV
SNR
PWN?
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Pulsar wind nebula
How many sources make up MGRO J2019+37?
We identified CTB87 and a large extended region
Brightness profile: 2 or 3 sources?
10 years VERITAS Jun 28-29, 2017
SNR
PWN?
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Gamma-ray binaries: HESS J0632-057
Originally an unidentified TeV source
Initial non-detection with VERITAS variability
Periodicity found in X rays, confirmed in g-rays
No detection yet in GeV band with Fermi LAT
10 years VERITAS Jun 28-29, 2017
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Gamma-ray binaries: HESS J0632-057
Correlated variability in X rays and TeV gamma rays
Two peaks in light curve … an effect of orbit eccentricity?
Why peaks here?
10 years VERITAS Jun 28-29, 2017
X rays vs. TeV gamma rays
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Gamma-ray binaries: LS I +61 303
A B0 Ve 25 star
and
a compact object
10 years VERITAS Jun 28-29, 2017
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Gamma-ray binaries: LS I +61 303
10 years VERITAS Jun 28-29, 2017
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Gamma-ray binaries: LS I +61 303
A massive B0 Ve 25 star and a compact object
Nightly TeV variability
Uncorrelated
GeV and TeV emission
GeV spectrum similar
to that of a pulsar
10 years VERITAS Jun 28-29, 2017
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Gamma-ray binaries: LS I +61 303
Baseline TeV emission seen throughout entire orbit
Strong gamma-ray flares in some orbits
Little spectral variation
10 years VERITAS Jun 28-29, 2017
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Gamma-ray binaries: TeV J2032+4130
First unidentified TeV source (1990s, HEGRA)
2014: Association with pulsar
A pulsar wind nebula? Fits to know pulsar wind nebulae
10 years VERITAS Jun 28-29, 2017
g-ray pulsar
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Gamma-ray binaries : TeV J2032+4130
A possible partner in a long-period binary
shortly approaching periastron
X-ray flux increases significantly
What will the gamma-ray flux do?
10 years VERITAS Jun 28-29, 2017
X rays (Swift)
(Lyne et al. 2015)
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Conclusion
10 years of VERITAS operation
• A rich harvest of Galactic science
• Fundamental advances in understanding
• Physics interpretation combines all messengers
• There is more to come …
10 years VERITAS Jun 28-29, 2017