Skip to main navigation
Skip to search
Skip to main content
University of Illinois Urbana-Champaign Home
LOGIN & Help
Home
Profiles
Research units
Research & Scholarship
Datasets
Honors
Press/Media
Activities
Search by expertise, name or affiliation
Non-thermal models for infrared flares from Sgr A∗
Eric Petersen,
Charles Gammie
Astronomy
Physics
National Center for Supercomputing Applications (NCSA)
Research output
:
Contribution to journal
›
Article
›
peer-review
Overview
Fingerprint
Fingerprint
Dive into the research topics of 'Non-thermal models for infrared flares from Sgr A∗'. Together they form a unique fingerprint.
Sort by
Weight
Alphabetically
Keyphrases
Thermal Model
100%
Near-infrared
100%
Sgr A*
100%
Flux Density
66%
Centroid
33%
High Flux Density
33%
Order of Magnitude
16%
Probability Density Function
16%
Near-infrared Spectrum
16%
Spectral Slope
16%
Low Flux Density
16%
Image Size
16%
Quiescent State
16%
Electron Distribution Function
16%
Very-long-baseline Interferometry
16%
Image Centroid
16%
Density Probability
16%
Relativistic Magnetohydrodynamics
16%
Magnetohydrodynamic Simulation
16%
Proper Motions
16%
Thermal Component
16%
Power-law Tail
16%
Magnetic Reconnection
16%
Near-infrared Image
16%
Infrared Interferometry
16%
Physics
Near Infrared
100%
Flux Density
87%
Interferometry
12%
Distribution Function
12%
Electron Distribution
12%
Very Long Base Interferometry
12%
Magnetohydrodynamic Simulation
12%
Proper Motion
12%