photometric observations of the cataclysmic variable star ip peg rakutou high school kasumi goto...
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![Page 1: Photometric observations of the cataclysmic variable star IP Peg Rakutou High School Kasumi Goto Ayano Terada](https://reader036.vdocuments.net/reader036/viewer/2022062511/5514db00550346b0478b5475/html5/thumbnails/1.jpg)
Photometric Photometric observations of the observations of the cataclysmic variable cataclysmic variable star IP Peg star IP Peg
Rakutou High SchoolRakutou High SchoolKasumi Goto Ayano TeradaKasumi Goto Ayano Terada
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The history of Our The history of Our observationsobservations
60cm telescope of HIDA observatory, 60cm telescope of HIDA observatory, September 23th of 2005 September 23th of 2005
40cm telescope of Kyoto University’s roof 40cm telescope of Kyoto University’s roof observatory, November 22nd of 2005observatory, November 22nd of 2005
→ → these clouded when eclipse.these clouded when eclipse.
December 23rd of 2006December 23rd of 2006 → → light curvelight curve → → inclination angle of orbitinclination angle of orbit → → angle of Hotspot with Companionangle of Hotspot with Companion
Couldn’t observe!!
![Page 3: Photometric observations of the cataclysmic variable star IP Peg Rakutou High School Kasumi Goto Ayano Terada](https://reader036.vdocuments.net/reader036/viewer/2022062511/5514db00550346b0478b5475/html5/thumbnails/3.jpg)
•The system of CVs
Central star
→ Compact Star with Accretion Disc.
Companion (red giant)
Hot Spot
→ Where gas flow on Accretion Disk
The orbital period → typically several hours
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ObservationObservation
Automatic observation exposure time 30 sec.
Dec 23rd of 2006, JT 18:53~21:25.
The 40cm telescope at Kyoto University roof observatory.
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AnalysisAnalysis
IRAF software → at Kyoto university Makali`i (Subaru image processing software) → at school. We obtained stellar magnitudes.
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The light curve simulationThe light curve simulation
Using IDL system At Department of Astronomy, Kyoto
University
The inclinations The angles of Hot Spot with companion
↓simulation
Simulation code is made by Mr. Sugiyasu.
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companion
Accretion Disc
公転軌道面公転軸
Line of sight
Inclination
Revolution axis
降着円盤
視線方向
Surface of revolution orbit
伴星
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Relationship of the companion star and the accretion disk, and Hot spot
Hot Spot
Companion Accretion Disc
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Ordinate: magnitude Abscissa: time (hours)
The influence by the companion
center of eclipse
Factor point
Beginning of cloudy
The light curve
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The inclination is 85°The angle of Hot Spot with the companion is 25°
•The simulation light curve
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The inclination is 90°The inclination is 90°The angle of the Hot Spot with the companion is 25°The angle of the Hot Spot with the companion is 25°
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ResultResult
The inclination is 85°
The angle of the Hot Spot
with the companion is 25°
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AcknowledgmentAcknowledgment
We thank staff of Department
of Astronomy, Kyoto University.