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dc.contributor.authorLieshout, Rik van
dc.contributor.authorRappaport, Saul
dc.date.accessioned2017-12-07T17:30:15Z
dc.date.available2017-12-07T17:30:15Z
dc.date.issued2017-08-02
dc.identifier.urihttps://www.repository.cam.ac.uk/handle/1810/270066
dc.description.abstractWe discuss a new class of exoplanets that appear to be emitting a tail of dusty effluents. These disintegrating planets are found close to their host stars and have very hot, and likely molten, surfaces. The properties of the dust should provide a direct probe of the constituent material of these rocky bodies.
dc.publisherSpringer International Publishing
dc.titleDisintegrating Rocky Exoplanets
dc.typeArticle
prism.endingPage19
prism.publicationDate2018
prism.startingPage1
dc.identifier.doi10.17863/CAM.12487
rioxxterms.versionofrecord10.1007/978-3-319-30648-3_15-2
rioxxterms.versionAM
rioxxterms.licenseref.urihttp://www.rioxx.net/licenses/all-rights-reserved
rioxxterms.licenseref.startdate2018
dc.publisher.urlhttp://dx.doi.org/10.1007/978-3-319-55333-7_15
rioxxterms.typeJournal Article/Review
pubs.funder-project-idEuropean Research Council (279973)
cam.issuedOnline2017-11-11
rioxxterms.freetoread.startdate2018-09-18


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