Light Curve Analysis Of Tt Oph And Uz Oph

Details Light Curve Analysis Of Tt Oph And Uz Oph Light Curve Analysis Of Tt Oph And Uz Oph

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21734211c&link_type=abstract

American Astronomical Society, AAS Meeting #217, #342.11; Bulletin of the American Astronomical Society, Vol. 43, 2011

Astronomy and Astrophysics

Astronomy

Scientific paper

TT Oph and UZ Oph are both classified in the GCVS as RV Tauri stars, pulsating variables with alternating deep and shallow minima. The literature indicates that the RV Tauri nature of these two stars is questionable. We have examined the AAVSO light curves of these objects for the eight year period of 2002-2010. We will present our analysis of the light curves and discuss how their recent behavior compares with past behavior as presented in the literature.
Support for this work was provided by the NSF PAARE program to South Carolina State University under award AST-0750814.

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