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Results #1-#10 of 17
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Fitting Cosmological Data AP DEDGP  [ Computer Program ]
  
Match Score:
100
Byline:
J. Moldenhauer, F. Cavanna, W. O'Toole, and W. Zimmerman
Post a comment | Relations
Measurements of the Alcock-Paczynski test, support the accelerated expansion of the universe (cosmic acceleration). The simulation allows users to compare and fit theoretical models…
  
Match Score:
100
Byline:
M. Clyburn
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The EJS Binary Star System with Lorentz Symmetry Violating Effects 3D Model illustrates the effects of violations in Lorentz symmetry to any detached binary star system. Lorentz…
Stellar Blackbody Radiation Curves  [ Computer Program ]
  
Match Score:
100
Byline:
M. Belloni
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The Stellar Blackbody Radiation Curves model simulates the blackbody radiation curve of stars and how this leads to the observed color and luminosity of the star. If a star can be…
Hertzsprung–Russell (H-R) Diagrams  [ Computer Program ]
  
Match Score:
100
Byline:
M. Belloni
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The Hertzsprung–Russell (H-R) Diagrams model simulates Hertzsprung–Russell (HR or H-R) diagram for groups of stars. The diagram is a scatter plot of steller luminosity vs. stellar…
Fitting Cosmological Supernovae Data DEDGP  [ Computer Program ]
  
Match Score:
100
Byline:
J. Moldenhauer, L. Engelhardt, and K. Stone
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The Fitting Cosmological Supernovae Data Model allows users to compare and fit cosmological models with recent supernovae type Ia datasets to confirm the accelerated expansion of the…
Pulsar Sounds Audio Demonstration JS Model  [ Computer Program ]
  
Match Score:
100
Byline:
W. Christian and F. Esquembre
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The Pulsar Sounds Audio Demonstration Model plays audio recordings of various pulsars from within a JavaScript EjsS model. The Pulsar Sounds Audio Demonstration Model was…
Stellar Aberration 2D  [ Computer Program ]
  
Match Score:
100
Byline:
T. Timberlake
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The Stellar Aberration 2D Model illustrates the phenomenon known as the aberration of starlight, first reported by James Bradley in 1729. Aberration occurs because light has a finite…
Stellar Aberration 3D  [ Computer Program ]
  
Match Score:
100
Byline:
T. Timberlake
Post a comment | Relations
The Stellar Aberration 3D Model illustrates the phenomenon known as the aberration of starlight, first reported by James Bradley in 1729. Aberration occurs because light has a finite…
Shapley's Globular Clusters  [ Computer Program ]
  
Match Score:
100
Byline:
T. Timberlake
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The EJS Shapley's Globular Clusters Model shows the distribution of globular clusters around the plane of the Milky Way as determined by Harlow Shapley in 1918. The Space View frame…
Eclipsing Binary Stars  [ Computer Program ]
  
Match Score:
100
Byline:
M. Belloni
Post a comment | Relations
Eclipsing Binary Stars model simulates the detection of eclipsing binary stars. In this method, the light curve from the combination of the two stars, and how it changes over time…
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Results #1-#10 of 17

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