Irregular variable: Difference between revisions

Revision as of 16:42, 10 December 2009

Latest revision as of 18:03, 15 January 2024

(24 intermediate revisions by 20 users not shown)

Line 1:

{{Short description|Type of variable star}}

{{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.

'''Eruptive''' irregular variables are divided into three categories:

* Group I variables are split into subgroups IA (spectral types O to A) and IB (spectral types F through M).

* [[Orion variables]], GCVS type IN (irregular and nebulous), indigenous to star-forming regions, may vary by several magnitudes with rapid changes of up to 1 magnitude in 1 to 10 days, are similarly divided by spectral type into subgroups INA and INB, but with the addition of another subgroup, INT, for T Tauri stars, or INT(YY) for YY Orionis stars.

* Group I variables are split into subgroups IA (spectral types O to A) and IB (spectral types F through M).

* [[Orion variables]], GCVS type IN (irregular and nebulous), indigenous to star-forming regions, may vary by several magnitudes with rapid changes of up to 1 magnitude in 1 to 10 days, are similarly divided by spectral type into subgroups INA and INB, but with the addition of another subgroup, INT, for [[T Tauri starsstar]]s, or INT(YY) for YY Orionis stars.

* The third category of eruptive irregulars are the IS stars, which show rapid variations of 0.5 to 1 magnitude in a few hours or days; again, these come in subgroups ISA and ISB.

'''Pulsating''' irregular giants or supergiants, called [[slow irregular variable]]s, are all of late spectral types (K, M, C, or S), and classed as type L-LB for giants and LC for supergiants. How many of these are actually semi-regular variables that simply need more study, remains unclear.<ref>{{citation|title=Observing Variable Stars |author=Gerry Arlen Good|year= 2003|publisher=Springer Science|url= httphttps://books.google.com/books?vid=ISBN1852334983&id=k9ViYKvKRz0C&pg=PA8&lpg=PA8&ots=AojoVu3Lpn&dqq=%22Irregular+variable%22&iepg=ISO-8859-1&outputPA8|isbn=html&sig=hIF3ZDs978-Rh3XGKVECqONh7aKAYM|id=ISBN 1-85233-498-37}}</ref>

== References ==

{{Reflist}}

<references />

{{var-star-stub}}

[[Category:Irregular variables| ]]

[[ca:Estrella variable irregular]]

{{var-star-stub}}

[[es:Estrella variable irregular]]

[[eu:Izar aldagarri irregular]]

[[fr:Variable irrégulière]]

[[it:Variabile irregolare]]

[[pl:Gwiazda zmienna nieregularna]]

[[ru:Неправильные переменные звёзды]]

[[sk:Nepravidelná premenná hviezda]]

[[tr:Düzensiz değişen]]

[[zh:不規則變星]]