Alpha2 Canum Venaticorum variable
id:
alpha2-canum-venaticorum-variable-233-574873
title:
Alpha2 Canum Venaticorum variable
text:
An Alpha2 Canum Venaticorum variable is a type of variable star. These stars are chemically peculiar main sequence stars of spectral class B8p to A7p. They have strong magnetic fields and strong silicon, strontium, or chromium spectral lines. Their brightness typically varies by 0.01 to 0.1 magnitudes over the course of 0.5 to 160 days. In addition to their intensities, the intensities and profiles of the spectral lines of α2 CVn variables also vary, as do their magnetic fields. The periods of t
brand slug:
wiki
category slug:
encyclopedia
description:
Variable star type
original url:
https://en.wikipedia.org/wiki/Alpha2_Canum_Venaticorum_variable
date created:
date modified:
2024-01-12T23:47:53Z
main entity:
{"identifier":"Q1141942","url":"https://www.wikidata.org/entity/Q1141942"}
image:
{"content_url":"https://upload.wikimedia.org/wikipedia/commons/a/a5/Alpha2CVnLightCurve.png","width":1500,"height":975}
fields total:
13
integrity:
15