Irregular variable: Difference between revisions

Revision as of 00:26, 31 January 2021

Revision as of 10:12, 31 January 2021

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{{Proposed deletion/dated

|concern = I think this article should be replaced with a disambiguation page. As it is, I don't think it will ever become a very useful article because it merely contains short, jargon-rich and context-poor descriptions of members of a very heterogeneous class of stars. Each individual type of irregular variable deserves a decent article of its own, but having an article like this just seems confusing to me.

|timestamp = 20210131002642

|nom = PopePompus

|help = off

}}

{{Refimprove|date=December 2009}}

An '''irregular variable''' is a type of [[variable star]] in which variations in brightness show no regular [[Frequency|periodicity]]. There are two main sub-types of irregular variable: eruptive and pulsating.