A survey of hot subdwarf pulsators in ω Cen

We recently discovered an apparently new class of pulsating Extreme Horizontal Branch (EHB) star in ω Cen. Tightly clustered around ∼50,000 K, these H-rich sdO stars exhibit rapid, multi-periodic oscillations on a timescale of 100 s. While four such objects have been detected in ω Cen, no counterpar...

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Main Authors: Catelan M., Monelli M., Alonso M.L., Green E.M., Fontaine G., Calamida A., Randal S.K., Bono G., Dhillon V.S., Marsh T.R.
Format: Article
Language:English
Published: EDP Sciences 2013-03-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/20134304006
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author Catelan M.
Monelli M.
Alonso M.L.
Green E.M.
Fontaine G.
Calamida A.
Randal S.K.
Bono G.
Dhillon V.S.
Marsh T.R.
author_facet Catelan M.
Monelli M.
Alonso M.L.
Green E.M.
Fontaine G.
Calamida A.
Randal S.K.
Bono G.
Dhillon V.S.
Marsh T.R.
author_sort Catelan M.
collection DOAJ
description We recently discovered an apparently new class of pulsating Extreme Horizontal Branch (EHB) star in ω Cen. Tightly clustered around ∼50,000 K, these H-rich sdO stars exhibit rapid, multi-periodic oscillations on a timescale of 100 s. While four such objects have been detected in ω Cen, no counterparts have yet been found among the field population. Conversely, the rapid sdB pulsators around 31,000 K that are well-studied in the Galactic field have yet to be found in a globular cluster. We discuss the implications of this and also report the discovery of a fifth EHB pulsator in ω Cen.
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spelling doaj.art-4dbf9d6a4cae41058cd63cf1bb9a00472022-12-21T16:43:04ZengEDP SciencesEPJ Web of Conferences2100-014X2013-03-01430400610.1051/epjconf/20134304006A survey of hot subdwarf pulsators in ω CenCatelan M.Monelli M.Alonso M.L.Green E.M.Fontaine G.Calamida A.Randal S.K.Bono G.Dhillon V.S.Marsh T.R.We recently discovered an apparently new class of pulsating Extreme Horizontal Branch (EHB) star in ω Cen. Tightly clustered around ∼50,000 K, these H-rich sdO stars exhibit rapid, multi-periodic oscillations on a timescale of 100 s. While four such objects have been detected in ω Cen, no counterparts have yet been found among the field population. Conversely, the rapid sdB pulsators around 31,000 K that are well-studied in the Galactic field have yet to be found in a globular cluster. We discuss the implications of this and also report the discovery of a fifth EHB pulsator in ω Cen.http://dx.doi.org/10.1051/epjconf/20134304006
spellingShingle Catelan M.
Monelli M.
Alonso M.L.
Green E.M.
Fontaine G.
Calamida A.
Randal S.K.
Bono G.
Dhillon V.S.
Marsh T.R.
A survey of hot subdwarf pulsators in ω Cen
EPJ Web of Conferences
title A survey of hot subdwarf pulsators in ω Cen
title_full A survey of hot subdwarf pulsators in ω Cen
title_fullStr A survey of hot subdwarf pulsators in ω Cen
title_full_unstemmed A survey of hot subdwarf pulsators in ω Cen
title_short A survey of hot subdwarf pulsators in ω Cen
title_sort survey of hot subdwarf pulsators in ω cen
url http://dx.doi.org/10.1051/epjconf/20134304006
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