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Optical Light Curve of Nova KT Eridani
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| Zeitschriftentitel: | Proceedings of the International Astronomical Union |
|---|---|
| Personen und Körperschaften: | , , |
| In: | Proceedings of the International Astronomical Union, 8, 2012, S290, S. 191-192 |
| Format: | E-Article |
| Sprache: | Englisch |
| veröffentlicht: |
Cambridge University Press (CUP)
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| Schlagwörter: |
| author_facet |
Chen, W. P. Hung, L. W. Walter, Fred Chen, W. P. Hung, L. W. Walter, Fred |
|---|---|
| author |
Chen, W. P. Hung, L. W. Walter, Fred |
| spellingShingle |
Chen, W. P. Hung, L. W. Walter, Fred Proceedings of the International Astronomical Union Optical Light Curve of Nova KT Eridani Astronomy and Astrophysics Space and Planetary Science |
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chen, w. p. |
| spelling |
Chen, W. P. Hung, L. W. Walter, Fred 1743-9213 1743-9221 Cambridge University Press (CUP) Astronomy and Astrophysics Space and Planetary Science http://dx.doi.org/10.1017/s1743921312019564 <jats:title>Abstract</jats:title><jats:p>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.</jats:p> Optical Light Curve of Nova KT Eridani Proceedings of the International Astronomical Union |
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| title |
Optical Light Curve of Nova KT Eridani |
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Optical Light Curve of Nova KT Eridani |
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Optical Light Curve of Nova KT Eridani |
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Optical Light Curve of Nova KT Eridani |
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Optical Light Curve of Nova KT Eridani |
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Optical Light Curve of Nova KT Eridani |
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optical light curve of nova kt eridani |
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Astronomy and Astrophysics Space and Planetary Science |
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http://dx.doi.org/10.1017/s1743921312019564 |
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2012 |
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191-192 |
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<jats:title>Abstract</jats:title><jats:p>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.</jats:p> |
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| author | Chen, W. P., Hung, L. W., Walter, Fred |
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| description | <jats:title>Abstract</jats:title><jats:p>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.</jats:p> |
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| imprint | Cambridge University Press (CUP), 2012 |
| imprint_str_mv | Cambridge University Press (CUP), 2012 |
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| spelling | Chen, W. P. Hung, L. W. Walter, Fred 1743-9213 1743-9221 Cambridge University Press (CUP) Astronomy and Astrophysics Space and Planetary Science http://dx.doi.org/10.1017/s1743921312019564 <jats:title>Abstract</jats:title><jats:p>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.</jats:p> Optical Light Curve of Nova KT Eridani Proceedings of the International Astronomical Union |
| spellingShingle | Chen, W. P., Hung, L. W., Walter, Fred, Proceedings of the International Astronomical Union, Optical Light Curve of Nova KT Eridani, Astronomy and Astrophysics, Space and Planetary Science |
| title | Optical Light Curve of Nova KT Eridani |
| title_full | Optical Light Curve of Nova KT Eridani |
| title_fullStr | Optical Light Curve of Nova KT Eridani |
| title_full_unstemmed | Optical Light Curve of Nova KT Eridani |
| title_short | Optical Light Curve of Nova KT Eridani |
| title_sort | optical light curve of nova kt eridani |
| title_unstemmed | Optical Light Curve of Nova KT Eridani |
| topic | Astronomy and Astrophysics, Space and Planetary Science |
| url | http://dx.doi.org/10.1017/s1743921312019564 |