About this document
Mass-to-Light Ratio in Globular Clusters by Max Eisenhardt is a document available to read on EtoBox.
1) The document provides information to calculate the mass-to-light ratio of a globular cluster. Using the given properties, the calculation determines the ratio is 1.47 solar masses per solar luminosity in the V-band. 2) Using a conversion from Kennicutt (1988), the calculation estimates the global star formation rate density of the universe today based on UV luminosity data from a galaxy survey to be 0.00506 solar masses per year per megaparsec cubed. 3) The document provides properties of the disk a
- Author
- Max Eisenhardt
- Language
- EN