KIC2569073, A second Cepheid in the Kepler FOV
One particularly interesting new variable discovered via Kepler’s 200x200 pixel superstamp images is KIC2569073. With a period of 14.66 days and 0.04mag variability it is only the second Cepheid in the Kepler field, or a rotationally modulated variable. We discuss its classification as a Type II W V...
| Main Authors: | , , , , |
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| Format: | Article |
| Language: | English |
| Published: |
EDP Sciences
2015-01-01
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| Series: | EPJ Web of Conferences |
| Online Access: | http://dx.doi.org/10.1051/epjconf/201510106024 |
| _version_ | 1818655189258731520 |
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| author | Drury Jason A. Kuehn Charles A. Bellamy Beau R. Stello Dennis Bedding Timothy R. |
| author_facet | Drury Jason A. Kuehn Charles A. Bellamy Beau R. Stello Dennis Bedding Timothy R. |
| author_sort | Drury Jason A. |
| collection | DOAJ |
| description | One particularly interesting new variable discovered via Kepler’s 200x200 pixel superstamp images is KIC2569073. With a period of 14.66 days and 0.04mag variability it is only the second Cepheid in the Kepler field, or a rotationally modulated variable. We discuss its classification as a Type II W Virginis Class Cepheid, and present the cycle-to-cycle period variations of this star, as well as the first direct observations of granulation noise within a Cepheid. |
| first_indexed | 2024-12-17T03:05:44Z |
| format | Article |
| id | doaj.art-6499af45d15f49869360a6b78e533028 |
| institution | Directory Open Access Journal |
| issn | 2100-014X |
| language | English |
| last_indexed | 2024-12-17T03:05:44Z |
| publishDate | 2015-01-01 |
| publisher | EDP Sciences |
| record_format | Article |
| series | EPJ Web of Conferences |
| spelling | doaj.art-6499af45d15f49869360a6b78e5330282022-12-21T22:05:57ZengEDP SciencesEPJ Web of Conferences2100-014X2015-01-011010602410.1051/epjconf/201510106024epjconf_sphr2014_06024KIC2569073, A second Cepheid in the Kepler FOVDrury Jason A.Kuehn Charles A.Bellamy Beau R.Stello DennisBedding Timothy R.One particularly interesting new variable discovered via Kepler’s 200x200 pixel superstamp images is KIC2569073. With a period of 14.66 days and 0.04mag variability it is only the second Cepheid in the Kepler field, or a rotationally modulated variable. We discuss its classification as a Type II W Virginis Class Cepheid, and present the cycle-to-cycle period variations of this star, as well as the first direct observations of granulation noise within a Cepheid.http://dx.doi.org/10.1051/epjconf/201510106024 |
| spellingShingle | Drury Jason A. Kuehn Charles A. Bellamy Beau R. Stello Dennis Bedding Timothy R. KIC2569073, A second Cepheid in the Kepler FOV EPJ Web of Conferences |
| title | KIC2569073, A second Cepheid in the Kepler FOV |
| title_full | KIC2569073, A second Cepheid in the Kepler FOV |
| title_fullStr | KIC2569073, A second Cepheid in the Kepler FOV |
| title_full_unstemmed | KIC2569073, A second Cepheid in the Kepler FOV |
| title_short | KIC2569073, A second Cepheid in the Kepler FOV |
| title_sort | kic2569073 a second cepheid in the kepler fov |
| url | http://dx.doi.org/10.1051/epjconf/201510106024 |
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