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Variable star light curves

   

Variable stars Deep-sky Asteroids Mars drawings About me First page

  A light curve it is used to study the brightness of a variable star in time. For a good light curve many observations are needed. The light curves from this page are made with my observations and may not be very accurate.

But for a variable star observer a light curve is something very special. It shows the observations made over a period of many years of observing.

The light curves from below were made by plotting the observed magnitude of the variable versus JD (Julian Date). Light curves updated on July 2004.

AGDra.html
AGDra
CHCyg.html
CHCyg
ChiCyg.html
ChiCyg
OmiCet.html
OmiCet
RCyg.html
RCyg
RDra.html
RDra
RLeo.html
RLeo
RSCyg.html
RSCyg
RTCyg.html
RTCyg
RTri.html
RTri
RUma.html
RUma
SCep.html
SCep
SSCyg.html
SSCyg
STAnd.html
STAnd
SUma.html
SUma
SUmi.html
SUmi
SVCas.html
SVCas
TCas.html
TCas
TCep.html
TCep
TCrb.html
TCrb
TUAnd.html
TUAnd
UCyg.html
UCyg
UOri.html
UOri
UPer.html
UPer
V838Mon.html
V838Mon
VCrb.html
VCrb
WCas.html
WCas
YPer.html
YPer
ZAnd.html
ZAnd

 

 

Other variable star pages

AAVSO - USA

VSNET - Japan

AFOEV - France

BAAVSS - England

BAV - Germany

MCSE - Hungary

RASNZ - Australia

Center for Backyard astrophysics CBA

Sirius Astronomy

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