FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3102682014> ?p ?o ?g. }

• W3102682014 endingPage "205" @default.
• W3102682014 startingPage "205" @default.
• W3102682014 abstract "Observations of nine transits of WASP-107 during the K2 mission reveal three separate occasions when the planet crossed in front of a starspot. The data confirm the stellar rotation period to be 17 days—approximately three times the planet's orbital period—and suggest that large spots persist for at least one full rotation. If the star had a low obliquity, at least two additional spot crossings should have been observed. They were not observed, giving evidence for a high obliquity. We use a simple geometric model to show that the obliquity is likely in the range 40°–140°, i.e., both spin–orbit alignment and anti-alignment can be ruled out. WASP-107 thereby joins the small collection of relatively low-mass stars with a high obliquity. Most such stars have been observed to have low obliquities; all of the exceptions, including WASP-107, involve planets with relatively wide orbits (warm Jupiters, with ). This demonstrates a connection between stellar obliquity and planet properties, in contradiction to some theories for obliquity excitation." @default.
• W3102682014 created "2020-11-23" @default.
• W3102682014 creator A5016187050 @default.
• W3102682014 creator A5064775419 @default.
• W3102682014 date "2017-04-08" @default.
• W3102682014 modified "2023-10-18" @default.
• W3102682014 title "The Oblique Orbit of WASP-107b from<i>K2</i>Photometry" @default.
• W3102682014 cites W1933520842 @default.
• W3102682014 cites W1955653533 @default.
• W3102682014 cites W1972674313 @default.
• W3102682014 cites W1974618482 @default.
• W3102682014 cites W1986316936 @default.
• W3102682014 cites W1992486633 @default.
• W3102682014 cites W2004802635 @default.
• W3102682014 cites W2012182714 @default.
• W3102682014 cites W2019263264 @default.
• W3102682014 cites W2024502805 @default.
• W3102682014 cites W2037349416 @default.
• W3102682014 cites W2038895269 @default.
• W3102682014 cites W2040091043 @default.
• W3102682014 cites W2043250362 @default.
• W3102682014 cites W2049260159 @default.
• W3102682014 cites W2105167493 @default.
• W3102682014 cites W2120949897 @default.
• W3102682014 cites W2130754528 @default.
• W3102682014 cites W2132117032 @default.
• W3102682014 cites W2133670009 @default.
• W3102682014 cites W2147406566 @default.
• W3102682014 cites W2170534558 @default.
• W3102682014 cites W2197396295 @default.
• W3102682014 cites W3098319597 @default.
• W3102682014 cites W3100585417 @default.
• W3102682014 cites W3101547990 @default.
• W3102682014 cites W3101662474 @default.
• W3102682014 cites W3102014803 @default.
• W3102682014 cites W3102113537 @default.
• W3102682014 cites W3102629466 @default.
• W3102682014 cites W3102998789 @default.
• W3102682014 cites W3103224716 @default.
• W3102682014 cites W3103290949 @default.
• W3102682014 cites W3104104914 @default.
• W3102682014 cites W3105218762 @default.
• W3102682014 cites W3105469181 @default.
• W3102682014 cites W3105621264 @default.
• W3102682014 cites W3105842161 @default.
• W3102682014 cites W3122233024 @default.
• W3102682014 cites W3124779831 @default.
• W3102682014 doi "https://doi.org/10.3847/1538-3881/aa65d1" @default.
• W3102682014 hasPublicationYear "2017" @default.
• W3102682014 type Work @default.
• W3102682014 sameAs 3102682014 @default.
• W3102682014 citedByCount "60" @default.
• W3102682014 countsByYear W31026820142017 @default.
• W3102682014 countsByYear W31026820142018 @default.
• W3102682014 countsByYear W31026820142019 @default.
• W3102682014 countsByYear W31026820142020 @default.
• W3102682014 countsByYear W31026820142021 @default.
• W3102682014 countsByYear W31026820142022 @default.
• W3102682014 countsByYear W31026820142023 @default.
• W3102682014 crossrefType "journal-article" @default.
• W3102682014 hasAuthorship W3102682014A5016187050 @default.
• W3102682014 hasAuthorship W3102682014A5064775419 @default.
• W3102682014 hasBestOaLocation W31026820141 @default.
• W3102682014 hasConcept C121332964 @default.
• W3102682014 hasConcept C127413603 @default.
• W3102682014 hasConcept C1276947 @default.
• W3102682014 hasConcept C146978453 @default.
• W3102682014 hasConcept C150846664 @default.
• W3102682014 hasConcept C196644772 @default.
• W3102682014 hasConcept C32161561 @default.
• W3102682014 hasConcept C44870925 @default.
• W3102682014 hasConcept C51244244 @default.
• W3102682014 hasConcept C68271606 @default.
• W3102682014 hasConcept C88991977 @default.
• W3102682014 hasConcept C9411552 @default.
• W3102682014 hasConceptScore W3102682014C121332964 @default.
• W3102682014 hasConceptScore W3102682014C127413603 @default.
• W3102682014 hasConceptScore W3102682014C1276947 @default.
• W3102682014 hasConceptScore W3102682014C146978453 @default.
• W3102682014 hasConceptScore W3102682014C150846664 @default.
• W3102682014 hasConceptScore W3102682014C196644772 @default.
• W3102682014 hasConceptScore W3102682014C32161561 @default.
• W3102682014 hasConceptScore W3102682014C44870925 @default.
• W3102682014 hasConceptScore W3102682014C51244244 @default.
• W3102682014 hasConceptScore W3102682014C68271606 @default.
• W3102682014 hasConceptScore W3102682014C88991977 @default.
• W3102682014 hasConceptScore W3102682014C9411552 @default.
• W3102682014 hasIssue "5" @default.
• W3102682014 hasLocation W31026820141 @default.
• W3102682014 hasLocation W31026820142 @default.
• W3102682014 hasLocation W31026820143 @default.
• W3102682014 hasOpenAccess W3102682014 @default.
• W3102682014 hasPrimaryLocation W31026820141 @default.
• W3102682014 hasRelatedWork W1533773444 @default.
• W3102682014 hasRelatedWork W2018181716 @default.
• W3102682014 hasRelatedWork W2072052661 @default.
• W3102682014 hasRelatedWork W2113930839 @default.
• W3102682014 hasRelatedWork W2317963360 @default.

• next