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Very High-energy Gamma-ray Emission from LS I +61° 303 Binary
VERITAS collaboration
Astronomy & Astrophysics
Center for Particle and Gravitational Astrophysics
Research output
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peer-review
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Dive into the research topics of 'Very High-energy Gamma-ray Emission from LS I +61° 303 Binary'. Together they form a unique fingerprint.
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Keyphrases
High Energy
100%
Gamma-ray Emission
100%
High-gamma
100%
LS I +61 303
100%
Orbital Period
75%
Spectral Energy Distribution
50%
Radio
50%
Compact Objects
50%
VERITAS
50%
Neutron Stars
25%
Source Type
25%
Imaging Atmospheric Cherenkov Telescope
25%
Energy Band
25%
Modulation Period
25%
Spectral Measurement
25%
At a Distance
25%
Absorption Mechanism
25%
Periodic Excitation
25%
Particle Acceleration
25%
TeV Energies
25%
Gamma-ray Sources
25%
Cherenkov Telescope Array
25%
Eccentric Orbits
25%
Black Holes-stars
25%
Acceleration Mechanism
25%
Gamma-ray Binaries
25%
Modulation Pattern
25%
Distribution Behavior
25%
Physics
Gamma Radiation
100%
Compact Objects
66%
Spectral Energy Distribution
66%
Neutron Stars
33%
Atmospherics
33%
Energy Band
33%
Eccentric Orbit
33%
Gamma-Ray Sources
33%
Particle Acceleration
33%
Black Hole
33%