Arp, Halton C. (1953) Variable stars with periods greater than one day in globular clusters. Dissertation (Ph.D.), California Institute of Technology. http://resolver.caltech.edu/CaltechETD:etd-05052003-160207
Nineteen variable stars with periods greater than one day were observed in six globular clusters. The observational techniques and the accuracy of the measurements are discussed and light curves for 15 variables are exhibited.
Color-magnitude diagrams for six clusters are presented and the distance modulus to each is derived.
The resulting period-luminosity relation for type II cepheids indicates there are actually three separate lines in the period-luminosity diagram which these variables occupy. Means of identifying stars on these different lines are presented. The factor of two in the period which these lines are from each other is discussed from the standpoint of the nature of cepheid variation. Finally a hypothesis is advanced to explain the connection between type I and type II cepheids.
|Item Type:||Thesis (Dissertation (Ph.D.))|
|Degree Grantor:||California Institute of Technology|
|Division:||Physics, Mathematics and Astronomy|
|Thesis Availability:||Public (worldwide access)|
|Defense Date:||1 January 1953|
|Default Usage Policy:||No commercial reproduction, distribution, display or performance rights in this work are provided.|
|Deposited By:||Imported from ETD-db|
|Deposited On:||06 May 2003|
|Last Modified:||26 Dec 2012 02:39|
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