THE EFFECT of VARIABILITY on X-RAY BINARY LUMINOSITY FUNCTIONS: MULTIPLE-EPOCH OBSERVATIONS of NGC 300 with CHANDRA

Keyphrases

• Luminosity Function 100%
• X-ray Binaries 100%
• Active Galactic nuclei 66%
• Simple Power Law 66%
• Power Law 66%
• Low-mass X-ray Binaries 66%
• Power-law Index 66%
• X-ray 33%
• Fainting 33%
• Outburst 33%
• Mass Transfer 33%
• Spiral Galaxies 33%
• High Heat Flux 33%
• Generative Models 33%
• Maximum Distribution 33%
• Point Source 33%
• Source Population 33%
• X-ray Sources 33%
• Overflow 33%
• X-ray Flux 33%
• Eddington 33%
• Differential Power 33%
• Eddington Luminosity 33%
• Roche Lobe 33%
• High-mass X-ray Binaries 33%

Physics

• Luminosity Function 100%
• X Ray Binaries 100%
• Low-Mass X-Ray Binary Stars 66%
• Active Galactic Nuclei 66%
• Optical Bursts 33%
• High-Mass X-Ray Binary Stars 33%
• Roche Lobe 33%
• Spiral Galaxy 33%
• X Ray Source 33%