| We present results from high speed photometry
of nova-like variables VY Scl stars,UX UMa stars and SW Sextantis stars.Some
nova-like are best known to show - low states - .or fading episodes.
In some systems, these low states occur very infrequentely- 400days. Such low states provide a unique opportunity to study the white-dwarf atmosphere. The duration between 300 and 400 days and depth > 2 mag are typical for VY Scl type fadings. Nosotros presentamos observaciones de estrellas de tipo VY Scl, UX UMa y SW Sextantis. algunas de estas estrellas tardan más de 400dias en pasar a su fase de mínimo. Cuando alcanza esta fase es cuando se pueden estudiar mejor la atmósfera de la nova enana. La duración entre 300 y 400 días y su caída de luz de > 2 magnitudes es el comportamiento estándar en este tipo de estrellas. References. T Kato (VSNET 2004) Greiner, 1998 |
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Low state (2005) |
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Low state(2005) |
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Low state (2005) |
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| SDSSJ075443+500729 |
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| HS0943+1404 | Low state (2007)
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Low state (2005)
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Low state (2006)
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Photometric Study |
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-20:46:50.3 |
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-03:39:50.8 |
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1898-1933
1958-1967 1985-2006 |
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UP-TO-DATE LINEAR ELEMENTS OF ECLIPSING BINARIES
Reporting your photometric error (AAVSO)/ Calculando el error en fotometría
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