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    • https://phys.libretexts.org/Courses/Georgia_State_University/GSU-TM-Introductory_Physics_II_(1112)/zz%3A_Back_Matter/10%3A_13.1%3A_Appendix_J-_Physics_Formulas_(Wevers)/1.16%3A_Astrophysics
      Astrophysics, stellar evolution and energy production
    • https://phys.libretexts.org/Learning_Objects/A_Physics_Formulary/Physics/16%3A_Astrophysics
      Astrophysics, stellar evolution and energy production
    • https://phys.libretexts.org/Bookshelves/Astronomy__Cosmology/Big_Ideas_in_Cosmology_(Coble_et_al.)/06%3A_Measuring_Cosmic_Distances/6.03%3A_Standard_Candle
      Where the line meets your chosen distance modulus you can read the corresponding distance by scanning horizontally over to find the value for distance on the vertical axis: The green line gives the di...Where the line meets your chosen distance modulus you can read the corresponding distance by scanning horizontally over to find the value for distance on the vertical axis: The green line gives the distance in parsecs, the blue line gives it in kiloparsecs and the red line gives the distance in megaparsecs.

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