RS Canum Venaticorum variable
id:
rs-canum-venaticorum-variable-175-3165361
title:
RS Canum Venaticorum variable
text:
An RS Canum Venaticorum variable is a type of variable star. The variable type consists of close binary stars having active chromospheres which can cause large stellar spots. These spots are believed to cause variations in their observed luminosity. Systems can exhibit variations on timescales of years due to variation in the spot surface coverage fraction, as well as periodic variations which are, in general, close to the orbital period of the binary system. Some systems exhibit variations in l
brand slug:
wiki
category slug:
encyclopedia
description:
original url:
https://en.wikipedia.org/wiki/RS_Canum_Venaticorum_variable
date created:
2005-09-20T05:14:30Z
date modified:
2024-09-03T00:57:57Z
main entity:
{"identifier":"Q1392913","url":"https://www.wikidata.org/entity/Q1392913"}
image:
{"content_url":"https://upload.wikimedia.org/wikipedia/commons/4/4b/RSCVnLightCurve.png","width":1500,"height":975}
fields total:
13
integrity:
15