Re-Ananlysis of CN Ori, UZ Ser and X Leo with Composite Accretion Disk plus Photosphere Models

Details Re-Ananlysis of CN Ori, UZ Ser and X Leo with Composite Accretion Disk plus Photosphere Models Re-Ananlysis of CN Ori, UZ Ser and X Leo with Composite Accretion Disk plus Photosphere Models

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aas...201.4012u&link_type=abstract

American Astronomical Society, 201st AAS Meeting, #40.12; Bulletin of the American Astronomical Society, Vol. 34, p.1163

Astronomy and Astrophysics

Astronomy

Scientific paper

We have carried out a further study of the behavior and physical properties of the dwarf novae UZ Ser, X Leo and CN Ori during quiescence, using archival IUE NEWSIPS spectra. Previous studies (Henry and Sion 2001; Urban et al. 2001) determined the best-fitting white dwarf models and best-fitting accretion disks to the quiecent spectra but did not use combinations of disks and photospheres along with the best distance estimates. We have re-ananlyzed the three systems with composite disk plus photosphere models and present the results along witht their implications.. This work was supported by NSF grant AST9901955 and a summer research grant from the NASA Delaware Space Grant Consortium

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