A survey of hot subdwarf pulsators in ω Cen
dc.catalogador | kjc | |
dc.contributor.author | Randal, S. K. | |
dc.contributor.author | Calamida, A. | |
dc.contributor.author | Fontaine, G. | |
dc.contributor.author | Green, E. M. | |
dc.contributor.author | Monelli, M. | |
dc.contributor.author | Alonso, M. L. | |
dc.contributor.author | Catelan , Marcio | |
dc.contributor.author | Bono, G. | |
dc.contributor.author | Dhillon, V. S. | |
dc.contributor.author | Marsh, T. R. | |
dc.date.accessioned | 2024-03-04T17:01:46Z | |
dc.date.available | 2024-03-04T17:01:46Z | |
dc.date.issued | 2013 | |
dc.description.abstract | 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.... | |
dc.fechaingreso.objetodigital | 2024-05-16 | |
dc.fuente.origen | ORCID | |
dc.identifier.doi | 10.1051/epjconf/20134304006 | |
dc.identifier.uri | https://doi.org/10.1051/epjconf/20134304006 | |
dc.identifier.uri | https://repositorio.uc.cl/handle/11534/83711 | |
dc.information.autoruc | Instituto de Astrofísica; Catelan , Marcio; 0000-0001-6003-8877; 1001556 | |
dc.language.iso | en | |
dc.nota.acceso | Contenido completo | |
dc.rights | acceso abierto | |
dc.title | A survey of hot subdwarf pulsators in ω Cen | |
dc.type | comunicación de congreso | |
sipa.codpersvinculados | 1001556 | |
sipa.trazabilidad | ORCID;2024-01-22 |
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