Lectures in The Nature of Stars
Lecture 1: Introduction
Lecture 2: What Is Apparent Magnitude?
Lecture 3: Apparent Magnitude: Example
Lecture 4: What Is Absolute Magnitude?
Lecture 5: Find Distance Given Absolute & Apparent Magnitude
Lecture 6: Find Distance Given Absolute & Apparent Magnitude
Lecture 7: Using Angle Of Parallax To Find Distances
Lecture 8: Using Angle Of Parallax To Find Distances
Lecture 9: Difference Between Luminosity And Power
Lecture 10: Relationship Between Intensity And Luminosity
Lecture 11: Difference Between Luminosity And Brightness
Lecture 12: Brightness Explained
Lecture 13: Luminosity And Brightness
Lecture 14: Apparent Magnitude: Another Look
Lecture 15: Comparing Luminosity
Lecture 16: What Is Bolometric Magnitude?
Lecture 17: Wien'S Law, Star'S Color And Temperature
Lecture 18: Ubv Photometry: Star Brightnessr And It'S Color
Lecture 19: Ubv Photometry: Examples Of Stars
Lecture 20: Ubv Photometry: Graphically
Lecture 21: Stellar Classification: Spectral Class
Lecture 22: Stellar Classification: Spectral Class
Lecture 23: Stellar Classification: Spectral Class
Lecture 24: Stellar Classification: Spectral Type
Lecture 25: Stellar Classification: Luminosity Class
Lecture 26: Stellar Classification: Examples
Lecture 27: Stellar Classification: Luminosity Class
Lecture 28: Determining A Star'S Luminosity
Lecture 29: Determining A Star'S Luminosity: Example
Lecture 30: Determining A Star'S Luminosity (Rigel)
Lecture 31: Determining Stellar Radii
Lecture 32: Determining Stellar Radii (Temperature Of Sirius)
Lecture 33: Determining Stellar Radii (Luminosity Of Sirius)
Lecture 34: Determining Stellar Radius Of Sirius
Lecture 35: Determining The Mass Of Of A Binary Star
Lecture 36: Determining The Mass Of Of A Binary Star: Example
Lecture 37: Mass-Luminosity Relationship