Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/23109
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | Guenther, E. W. | en_US |
dc.contributor.author | CUSANO, FELICE | en_US |
dc.contributor.author | Deeg, H. | en_US |
dc.contributor.author | Gandolfi, D. | en_US |
dc.contributor.author | Geier, S. | en_US |
dc.contributor.author | Grziwa, S. | en_US |
dc.contributor.author | Heber, U. | en_US |
dc.contributor.author | Tal-Or, L. | en_US |
dc.contributor.author | Sebastian, D. | en_US |
dc.contributor.author | Rodler, F. | en_US |
dc.date.accessioned | 2020-03-04T14:25:14Z | - |
dc.date.available | 2020-03-04T14:25:14Z | - |
dc.date.issued | 2015 | en_US |
dc.identifier.isbn | 9781510813342 | en_US |
dc.identifier.issn | 2101-6275 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/23109 | - |
dc.description.abstract | Although more than a thousand transiting extrasolar planets have been discovered, only very few of them orbit stars that are more massive than the Sun. The discovery of such planets is interesting, because they have formed in disks that are more massive but had a shorter life time than those of solar-like stars. Studies of planets more massive than the Sun thus tell us how the properties of the proto-planetary disks effect the formation of planets. Another aspect that makes these planets interesting is that they have kept their original orbital inclinations. By studying them we can thus find out whether the orbital axes planets are initially aligned to the stars rotational axes, or not. Here we report on the discovery of a planet of a 1.4 solar-mass star with a period of 5.6 days in a polar orbit made by CoRoT. This new planet thus is one of the few known close-in planets orbiting a star that is substantially more massive than the Sun. <P /> | en_US |
dc.language.iso | eng | en_US |
dc.title | A planet in a polar orbit of 1.4 solar-mass star | en_US |
dc.type | Conference paper | - |
dc.identifier.doi | 10.1051/epjconf/201510102001 | en_US |
dc.identifier.scopus | 2-s2.0-84960192316 | en_US |
dc.identifier.isi | 000372491300017 | en_US |
dc.identifier.url | https://www.epj-conferences.org/articles/epjconf/abs/2015/20/epjconf_sphr2014_02001/epjconf_sphr2014_02001.html | en_US |
dc.relation.medium | ELETTRONICO | en_US |
dc.relation.volume | 101 | en_US |
dc.relation.firstpage | 02001 | en_US |
dc.relation.numberofpages | 4 | en_US |
dc.type.referee | REF_4 | en_US |
dc.description.international | sì | en_US |
dc.relation.alleditors | García. R.A.; Ballot, J. | en_US |
dc.relation.ispartofbook | The Space Photometry Revolution - CoRoT Symposium 3, Kepler KASC-7 Joint Meeting | en_US |
dc.publisher.name | EDP Sciences | en_US |
dc.type.invited | no | en_US |
dc.relation.conferencename | The Space Photometry Revolution - CoRoT Symposium 3, Kepler KASC-7 Joint Meeting | en_US |
dc.relation.conferenceplace | Toulouse, France | en_US |
dc.relation.conferencedate | July 6-11, 2014 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | EPJ WEB OF CONFERENCES | en_US |
dc.type.miur | 273 Contributo in Atti di convegno | - |
dc.identifier.adsbibcode | 2015EPJWC.10102001G | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.cerifentitytype | Publications | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.grantfulltext | open | - |
item.languageiso639-1 | en | - |
item.openairetype | Conference paper | - |
crisitem.journal.journalissn | 2101-6275 | - |
crisitem.journal.ance | E201294 | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.orcid | 0000-0003-2910-6565 | - |
È visualizzato nelle collezioni: | 3.01 Contributi in Atti di convegno |
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