Faint variable stars observed with Kepler
We present preliminary analysis of approximately 10 variable stars observed with Kepler. The sample stars are faint, and have temperatures greater than 8000 K. The stars were observed for up to three quarters (Q14-Q16) in long cadence mode. Frequencies were extracted with Period04, and 1-21 frequenc...
| Main Authors: | , |
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| Format: | Article |
| Language: | English |
| Published: |
EDP Sciences
2017-01-01
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| Series: | EPJ Web of Conferences |
| Online Access: | https://doi.org/10.1051/epjconf/201715206004 |
| _version_ | 1819124967272349696 |
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| author | Lovekin Catherine Tompkins Jasmin |
| author_facet | Lovekin Catherine Tompkins Jasmin |
| author_sort | Lovekin Catherine |
| collection | DOAJ |
| description | We present preliminary analysis of approximately 10 variable stars observed with Kepler. The sample stars are faint, and have temperatures greater than 8000 K. The stars were observed for up to three quarters (Q14-Q16) in long cadence mode. Frequencies were extracted with Period04, and 1-21 frequencies were detected in each quarter, with an average of 8 frequencies per quarter. Some variability is detected from quarter to quarter, while the dominant frequencies remain unchanged. We fit the frequencies using MESA models between 1.5 and 3 solar masses, and varied the core overshoot. Best fitting properties of each of these stars will be discussed. |
| first_indexed | 2024-12-22T07:32:39Z |
| format | Article |
| id | doaj.art-a01911bb2d9342d8ac7dadbca637272f |
| institution | Directory Open Access Journal |
| issn | 2100-014X |
| language | English |
| last_indexed | 2024-12-22T07:32:39Z |
| publishDate | 2017-01-01 |
| publisher | EDP Sciences |
| record_format | Article |
| series | EPJ Web of Conferences |
| spelling | doaj.art-a01911bb2d9342d8ac7dadbca637272f2022-12-21T18:33:58ZengEDP SciencesEPJ Web of Conferences2100-014X2017-01-011520600410.1051/epjconf/201715206004epjconf_puls2017_06004Faint variable stars observed with KeplerLovekin Catherine0Tompkins Jasmin1Physics Department, Mount Allison UniversityPhysics Department, Mount Allison UniversityWe present preliminary analysis of approximately 10 variable stars observed with Kepler. The sample stars are faint, and have temperatures greater than 8000 K. The stars were observed for up to three quarters (Q14-Q16) in long cadence mode. Frequencies were extracted with Period04, and 1-21 frequencies were detected in each quarter, with an average of 8 frequencies per quarter. Some variability is detected from quarter to quarter, while the dominant frequencies remain unchanged. We fit the frequencies using MESA models between 1.5 and 3 solar masses, and varied the core overshoot. Best fitting properties of each of these stars will be discussed.https://doi.org/10.1051/epjconf/201715206004 |
| spellingShingle | Lovekin Catherine Tompkins Jasmin Faint variable stars observed with Kepler EPJ Web of Conferences |
| title | Faint variable stars observed with Kepler |
| title_full | Faint variable stars observed with Kepler |
| title_fullStr | Faint variable stars observed with Kepler |
| title_full_unstemmed | Faint variable stars observed with Kepler |
| title_short | Faint variable stars observed with Kepler |
| title_sort | faint variable stars observed with kepler |
| url | https://doi.org/10.1051/epjconf/201715206004 |
| work_keys_str_mv | AT lovekincatherine faintvariablestarsobservedwithkepler AT tompkinsjasmin faintvariablestarsobservedwithkepler |