@inproceedings{82ad2b6b61f04072981f6bc3ce64aed2,
title = "Optical light curve of nova KT Eridani",
abstract = "We present the optical light curve of the very fast nova, KT Eridani, from its outburst in November 2009 to quiescence in 2012. Comparison of our data with the 24-hour monitoring by Swift on 2010 March 31 indicates a possible anticorrelation between the X-ray and optical emissions. A period of 57 d is found in the long-term optical light curve, which we interpret as the orbital modulation of the hot spot on the white dwarf disk accreting material from an early K-type giant. Our study lends support to the notation that KT Eri may be a recurrent nova.",
keywords = "Accretion disks, binaries: close, novae, white dwarfs, X-rays: binaries",
author = "Chen, {W. P.} and Hung, {L. W.} and Fred Walter",
year = "2012",
month = aug,
doi = "10.1017/S1743921312019564",
language = "???core.languages.en_GB???",
isbn = "9781107033795",
series = "Proceedings of the International Astronomical Union",
number = "S290",
pages = "191--192",
editor = "Chengmin Zhang and Tomaso Belloni and Mariano Mendez and Shuangnan Zhang",
booktitle = "Feeding Compact Objects",
edition = "S290",
}
