Hot spot in eclipsing dwarf nova iy ursae majoris during quiescence and normal outburst
Authors:
- Karolina Bąkowska,
- A. Olech
Abstract
We present the analysis of hot spot brightness in light curves of the eclipsing dwarf nova IY UMa during its normal outburst in March 2013 and in quiescence in April 2012 and in October 2015. Examination of four reconstructed light curves of the hot spot eclipses showed directly that the brightness of the hot spot changed significantly only during the outburst. The brightness of the hot spot, before and after the outburst, was on the same level. Thus, based on the behavior of the hot spot, IY UMa during its normal outburst follows the disk-instability model.
- Record ID
- UAM027da2aab2aa4c2e97f311a07c7b7ac8
- Author
- Journal series
- Acta Astronomica, ISSN 0001-5237
- Issue year
- 2015
- Vol
- 65
- Pages
- 351-360
- ASJC Classification
- ;
- Language
- (en) English
- Score (nominal)
- 30
- Score source
- journalList
- Score
- Publication indicators
- = 1; = 1; : 2015 = 0.810; : 2015 (2 years) = 2.000 - 2015 (5 years) =2.319
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- Uniform Resource Identifier
- https://researchportal.amu.edu.pl/info/article/UAM027da2aab2aa4c2e97f311a07c7b7ac8/
- URN
urn:amu-prod:UAM027da2aab2aa4c2e97f311a07c7b7ac8
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