Asteroseismology of Pulsating sdB Stars Observed at Catania Astrophysical Observatory
We present analysis of the data collected during three years of photometric campaigns at the 91 cm Cassegrain telescope of the Catania Astrophysical Observatory to observe the pulsating subdwarf B star PG 1336-018. For this eclipsing binary system, we obtained a precise determination of the orbital...
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Format: | Article |
Language: | English |
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De Gruyter
2003-06-01
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Series: | Open Astronomy |
Online Access: | https://doi.org/10.1515/astro-2017-0052 |
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author | Bonanno A. Frasca A. Lanza A. F. Ventura R. Mignemi B. Silvotti R. |
author_facet | Bonanno A. Frasca A. Lanza A. F. Ventura R. Mignemi B. Silvotti R. |
author_sort | Bonanno A. |
collection | DOAJ |
description | We present analysis of the data collected during three years of photometric campaigns at the 91 cm Cassegrain telescope of the Catania Astrophysical Observatory to observe the pulsating subdwarf B star PG 1336-018. For this eclipsing binary system, we obtained a precise determination of the orbital period which turns out to be P = 0.10101599±0.00000002 days. Time-series photometry reveals pulsation periods near 174 and 184 seconds. We also discuss a preliminary analysis of the data obtained in 2002 for the pulsating subdwarf PG 1325+101. |
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format | Article |
id | doaj.art-46fa08141f98437aa220c48438763010 |
institution | Directory Open Access Journal |
issn | 2543-6376 |
language | English |
last_indexed | 2024-12-17T05:43:39Z |
publishDate | 2003-06-01 |
publisher | De Gruyter |
record_format | Article |
series | Open Astronomy |
spelling | doaj.art-46fa08141f98437aa220c484387630102022-12-21T22:01:22ZengDe GruyterOpen Astronomy2543-63762003-06-0112228729410.1515/astro-2017-0052astro-2017-0052Asteroseismology of Pulsating sdB Stars Observed at Catania Astrophysical ObservatoryBonanno A.0Frasca A.1Lanza A. F.2Ventura R.3Mignemi B.4Silvotti R.5INAF – Osservatorio Astrofisico di Catania, Via S.Sofia 78, I-95123, Catania, ItalyINAF – Osservatorio Astrofisico di Catania, Via S.Sofia 78, I-95123, Catania, ItalyINAF – Osservatorio Astrofisico di Catania, Via S.Sofia 78, I-95123, Catania, ItalyINAF – Osservatorio Astrofisico di Catania, Via S.Sofia 78, I-95123, Catania, ItalyINAF – Osservatorio Astrofisico di Catania, Via S.Sofia 78, I-95123, Catania, ItalyOsservatorio Astronomico di Capodimonte, via Moiariello, 16 I-80131, Napoli, ItalyWe present analysis of the data collected during three years of photometric campaigns at the 91 cm Cassegrain telescope of the Catania Astrophysical Observatory to observe the pulsating subdwarf B star PG 1336-018. For this eclipsing binary system, we obtained a precise determination of the orbital period which turns out to be P = 0.10101599±0.00000002 days. Time-series photometry reveals pulsation periods near 174 and 184 seconds. We also discuss a preliminary analysis of the data obtained in 2002 for the pulsating subdwarf PG 1325+101.https://doi.org/10.1515/astro-2017-0052 |
spellingShingle | Bonanno A. Frasca A. Lanza A. F. Ventura R. Mignemi B. Silvotti R. Asteroseismology of Pulsating sdB Stars Observed at Catania Astrophysical Observatory Open Astronomy |
title | Asteroseismology of Pulsating sdB Stars Observed at Catania Astrophysical Observatory |
title_full | Asteroseismology of Pulsating sdB Stars Observed at Catania Astrophysical Observatory |
title_fullStr | Asteroseismology of Pulsating sdB Stars Observed at Catania Astrophysical Observatory |
title_full_unstemmed | Asteroseismology of Pulsating sdB Stars Observed at Catania Astrophysical Observatory |
title_short | Asteroseismology of Pulsating sdB Stars Observed at Catania Astrophysical Observatory |
title_sort | asteroseismology of pulsating sdb stars observed at catania astrophysical observatory |
url | https://doi.org/10.1515/astro-2017-0052 |
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