Pulsations in subdwarf B stars

Overview of attention for article published in Journal of Astrophysics and Astronomy, June 2005

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So far, Altmetric has seen 23 citations on 23 Wikipedia pages.

Swedish

V391 Pegasi

Cited by user Hans Frörum on 02 Jan 2024

V391 Pegasi eller HS 2201+2610 är en ensam stjärna belägen i den mellersta delen av stjärnbilden Pegasus.

Japanese

ペガスス座V391星

Cited by user Ringdownrabbit on 20 Jul 2019

German

Heißer Unterzwerg

Cited by user McBayne on 19 May 2018

Russian

Субкарлик спектрального класса B

Cited by user A Veselova on 02 Jul 2017

Arabic

نجم B شبه قزم

Cited by user Thedreammurad on 23 Mar 2017

French

Étoile sous-naine de type B

Cited by user 193.49.226.228 on 07 Mar 2017

Ukrainian

Субкарлик спектрального класу B

Cited by user Bilyavchyk on 27 Nov 2016

Czech

Podtrpaslík typu B

Cited by user Rottweiler on 16 Oct 2016

Chinese

B型次矮星

Cited by user SSR2000 on 04 May 2013

Chinese

飛馬座V391

Cited by user SSR2000 on 05 Jan 2013

Catalan

Estel subnan B

Cited by user Jagons on 14 Oct 2012

Portuguese

Estrela subanã B

Cited by user Romullo on 08 Aug 2011

Portuguese

Estrela subanã

Cited by user Romullo on 06 Aug 2011

Korean

페가수스자리 V391

Cited by user Ta183ta on 19 Jun 2010

Korean

B형 준왜성

Cited by user Rein7607 on 16 Jun 2010

Japanese

準矮星

Cited by user Punu on 16 Oct 2009

Japanese

B型準矮星

Cited by user Punu on 16 Oct 2009

Greek

Υπονάνος

Cited by user V-astro on 05 Sep 2009

Chinese

次矮星

Cited by user 凌雲 on 03 Sep 2009

German

Unterzwerg

Cited by user Arnomane on 13 Jun 2009

Italian

V391 Pegasi

Cited by user Roberto Mura on 26 Sep 2008

English

Subdwarf B star

Cited by user DOI bot on 11 Jun 2008

A B-type subdwarf (sdB) is a kind of subdwarf star with spectral type B. They differ from the typical subdwarf by being much hotter and brighter.

English

V391 Pegasi

Cited by user DOI bot on 09 Jun 2008

V391 Pegasi, also catalogued as HS 2201+2610, is a blue-white subdwarf star approximately 4,570 light-years away in the constellation of Pegasus.