K2ᅠReveals Pulsed Accretion Driven by the 2 Myr Old Hot Jupiter CI Tau b
dc.citation.articleNumber | L34 | en_US |
dc.citation.journalTitle | The Astrophysical Journal Letters | en_US |
dc.citation.volumeNumber | 853 | en_US |
dc.contributor.author | Biddle, Lauren I. | en_US |
dc.contributor.author | Johns-Krull, Christopher M. | en_US |
dc.contributor.author | Llama, Joe | en_US |
dc.contributor.author | Prato, Lisa | en_US |
dc.contributor.author | Skiff, Brian A. | en_US |
dc.date.accessioned | 2018-07-11T17:18:37Z | en_US |
dc.date.available | 2018-07-11T17:18:37Z | en_US |
dc.date.issued | 2018 | en_US |
dc.description.abstract | CIᅠTau is a young (~2 Myr) classical T Tauri star located in the Taurus star-forming region. Radial velocity observations indicate it hosts a Jupiter-sized planet with an orbital period of approximately 9 days. In this work, we analyze time series of CIᅠTau's photometric variability as seen byᅠK2. The light curve reveals the stellar rotation period to be ~6.6 days. Although there is no evidence that CIᅠTau b transits the host star, a ~9 day signature is also present in the light curve. We believe this is most likely caused by planetヨdisk interactions that perturb the accretion flow onto the star, resulting in a periodic modulation of the brightness with the ~9 day period of the planet's orbit. | en_US |
dc.identifier.citation | Biddle, Lauren I., Johns-Krull, Christopher M., Llama, Joe, et al.. "K2ᅠReveals Pulsed Accretion Driven by the 2 Myr Old Hot Jupiter CI Tau b." <i>The Astrophysical Journal Letters,</i> 853, (2018) IOP Publishing: https://doi.org/10.3847/2041-8213/aaa897. | en_US |
dc.identifier.doi | https://doi.org/10.3847/2041-8213/aaa897 | en_US |
dc.identifier.uri | https://hdl.handle.net/1911/102386 | en_US |
dc.language.iso | eng | en_US |
dc.publisher | IOP Publishing | en_US |
dc.rights | Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. | en_US |
dc.title | K2ᅠReveals Pulsed Accretion Driven by the 2 Myr Old Hot Jupiter CI Tau b | en_US |
dc.type | Journal article | en_US |
dc.type.dcmi | Text | en_US |
dc.type.publication | publisher version | en_US |
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