{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2022,4,2]],"date-time":"2022-04-02T13:48:51Z","timestamp":1648907331197},"reference-count":3,"publisher":"Cambridge University Press (CUP)","issue":"S282","license":[{"start":{"date-parts":[[2012,4,23]],"date-time":"2012-04-23T00:00:00Z","timestamp":1335139200000},"content-version":"unspecified","delay-in-days":297,"URL":"https:\/\/www.cambridge.org\/core\/terms"}],"content-domain":{"domain":[],"crossmark-restriction":false},"short-container-title":["Proc. IAU"],"published-print":{"date-parts":[[2011,7]]},"abstract":"<jats:title>Abstract<\/jats:title><jats:p>To date, there are several reported exoplanet detections within binary star systems. These findings are based on radial velocity data for the target star. However, the companion star could in turn have a companion of which we are not aware. We describe how this hidden binary system affects the radial velocity of the target star, mimicking a planet in some circumstances We also explain what can be done in practice in order to distinguish between these two effects.<\/jats:p>","DOI":"10.1017\/s1743921311027207","type":"journal-article","created":{"date-parts":[[2012,4,23]],"date-time":"2012-04-23T14:17:45Z","timestamp":1335190665000},"page":"137-138","source":"Crossref","is-referenced-by-count":0,"title":["Stellar Wobble Due to a Nearby Binary System"],"prefix":"10.1017","volume":"7","author":[{"given":"M. H. M.","family":"Morais","sequence":"first","affiliation":[]},{"given":"A. C. M.","family":"Correia","sequence":"additional","affiliation":[]}],"member":"56","published-online":{"date-parts":[[2012,4,23]]},"reference":[{"key":"S1743921311027207_ref1","first-page":"899","volume":"391","author":"Morais","year":"2008","journal-title":"AandA"},{"key":"S1743921311027207_ref2","first-page":"A152","volume":"525","author":"Morais","year":"2011","journal-title":"AandA"},{"key":"S1743921311027207_ref3","unstructured":"[3] Morais M. H. M. & Correia A. C. M. 2011, MNRAS, submitted"}],"container-title":["Proceedings of the International Astronomical Union"],"original-title":[],"language":"en","link":[{"URL":"https:\/\/www.cambridge.org\/core\/services\/aop-cambridge-core\/content\/view\/S1743921311027207","content-type":"unspecified","content-version":"vor","intended-application":"similarity-checking"}],"deposited":{"date-parts":[[2019,4,27]],"date-time":"2019-04-27T08:13:10Z","timestamp":1556352790000},"score":1,"resource":{"primary":{"URL":"https:\/\/www.cambridge.org\/core\/product\/identifier\/S1743921311027207\/type\/journal_article"}},"subtitle":[],"short-title":[],"issued":{"date-parts":[[2011,7]]},"references-count":3,"journal-issue":{"issue":"S282","published-print":{"date-parts":[[2011,7]]}},"alternative-id":["S1743921311027207"],"URL":"https:\/\/doi.org\/10.1017\/s1743921311027207","relation":{},"ISSN":["1743-9213","1743-9221"],"issn-type":[{"value":"1743-9213","type":"print"},{"value":"1743-9221","type":"electronic"}],"subject":[],"published":{"date-parts":[[2011,7]]}}}