Multi-site, multi-colour and space photometry of a southern δ Scuti star, 38 Eri
38 Eri is a δ Scuti star in the shell hydrogen burning stage of evolution, with a 0.04 mag peak-to-peak amplitude and a very complex light variation. It was discovered in 1971. In the subsequent investigation the star always showed a different frequency content. A ground-based multi-site campaign an...
| Main Authors: | , |
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| Format: | Article |
| Language: | English |
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EDP Sciences
2017-01-01
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| Series: | EPJ Web of Conferences |
| Online Access: | https://doi.org/10.1051/epjconf/201715205009 |
| _version_ | 1830357217414479872 |
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| author | Paparó Margit Benkö József |
| author_facet | Paparó Margit Benkö József |
| author_sort | Paparó Margit |
| collection | DOAJ |
| description | 38 Eri is a δ Scuti star in the shell hydrogen burning stage of evolution, with a 0.04 mag peak-to-peak amplitude and a very complex light variation. It was discovered in 1971. In the subsequent investigation the star always showed a different frequency content. A ground-based multi-site campaign and a MOST observation were devoted to resolve the contradicting pulsational behaviour. We present the preliminary result of our investigation obtained on Stromgren b and MOST data. The complexity of the pulsation is confirmed, but the comprehensive analysis helps to resolve the frequencies of the fast rotating star. |
| first_indexed | 2024-12-20T02:19:41Z |
| format | Article |
| id | doaj.art-57a15208aafc4364b82f6f2c514dd33d |
| institution | Directory Open Access Journal |
| issn | 2100-014X |
| language | English |
| last_indexed | 2024-12-20T02:19:41Z |
| publishDate | 2017-01-01 |
| publisher | EDP Sciences |
| record_format | Article |
| series | EPJ Web of Conferences |
| spelling | doaj.art-57a15208aafc4364b82f6f2c514dd33d2022-12-21T19:56:50ZengEDP SciencesEPJ Web of Conferences2100-014X2017-01-011520500910.1051/epjconf/201715205009epjconf_puls2017_05009Multi-site, multi-colour and space photometry of a southern δ Scuti star, 38 EriPaparó Margit0Benkö József1Konkoly Observatory, MTA CSFKKonkoly Observatory, MTA CSFK38 Eri is a δ Scuti star in the shell hydrogen burning stage of evolution, with a 0.04 mag peak-to-peak amplitude and a very complex light variation. It was discovered in 1971. In the subsequent investigation the star always showed a different frequency content. A ground-based multi-site campaign and a MOST observation were devoted to resolve the contradicting pulsational behaviour. We present the preliminary result of our investigation obtained on Stromgren b and MOST data. The complexity of the pulsation is confirmed, but the comprehensive analysis helps to resolve the frequencies of the fast rotating star.https://doi.org/10.1051/epjconf/201715205009 |
| spellingShingle | Paparó Margit Benkö József Multi-site, multi-colour and space photometry of a southern δ Scuti star, 38 Eri EPJ Web of Conferences |
| title | Multi-site, multi-colour and space photometry of a southern δ Scuti star, 38 Eri |
| title_full | Multi-site, multi-colour and space photometry of a southern δ Scuti star, 38 Eri |
| title_fullStr | Multi-site, multi-colour and space photometry of a southern δ Scuti star, 38 Eri |
| title_full_unstemmed | Multi-site, multi-colour and space photometry of a southern δ Scuti star, 38 Eri |
| title_short | Multi-site, multi-colour and space photometry of a southern δ Scuti star, 38 Eri |
| title_sort | multi site multi colour and space photometry of a southern δ scuti star 38 eri |
| url | https://doi.org/10.1051/epjconf/201715205009 |
| work_keys_str_mv | AT paparomargit multisitemulticolourandspacephotometryofasoutherndscutistar38eri AT benkojozsef multisitemulticolourandspacephotometryofasoutherndscutistar38eri |