Graduation Year

2011

Date of Thesis Acceptance

Fall 5-11-2011

Major Department or Program

Physics - Astronomy

Advisor(s)

Nathaniel Paust

Abstract

We present new BVI observations of the Galactic globular cluster M15. The observations cover an area 25 arcminutes square centered on the cluster. The color- magnitude diagram contains over 40,000 stars and extensive artificial star tests were performed to produce luminosity functions. The data extends from the tip of the red giant branch to below the main sequence turnoff. We compare the color-magnitude diagrams and RGB luminosity functions to Dartmouth Stellar Evolution Program (DSEP) models. Using an alpha abundance of [α/Fe] = 0.2 and a metallicity of [Fe/H] = −2.10 we find an age of 14.0 ± 1.0 Gyr and distance modulus of (m−M)V = 15.3 ± 0.1 through isochrone fitting. We find good agreement between the CMD fit and the fit to the luminosity functions.

Page Count

18

Subject Headings

Red giants, Stars -- Globular clusters, Whitman College 2011 -- Dissertation collection -- Physics-Astronomy

Permanent URL

http://hdl.handle.net/10349/1010

Document Type

Whitman Community Accessible Thesis

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