Magnetic Cataclysmic Variables
| dc.contributor.author | Kalomeni, Belinda | |
| dc.coverage.doi | 10.1063/1.3536370 | |
| dc.date.accessioned | 2016-12-13T11:37:31Z | |
| dc.date.available | 2016-12-13T11:37:31Z | |
| dc.date.issued | 2010 | |
| dc.description | International Conference on Binaries: In Celebration of Ron Webbink's 65th Birthday; Mykonos; Greece; 22 June 2010 through 25 June 2010 | en_US |
| dc.description.abstract | We present a study on magnetic cataclysmic variables (polars) using the collected data from the literature. These parameters (mass, radius, magnetic field intensity, mass transfer rate, etc.) and the relations between them are important to understand their nature, to explain the observed properties of them and to test the current evolutionary models. © 2010 American Institute of Physics. | en_US |
| dc.description.sponsorship | TÜBİTAK (Project No:109T047) and EBİLTEM | en_US |
| dc.identifier.citation | Kalomeni, B. (2010). Magnetic cataclysmic variables. AIP Conference Proceedings, 1314, 210-211. doi:10.1063/1.3536370 | en_US |
| dc.identifier.doi | 10.1063/1.3536370 | en_US |
| dc.identifier.doi | 10.1063/1.3536370 | |
| dc.identifier.isbn | 9780735408692 | |
| dc.identifier.issn | 0094-243X | |
| dc.identifier.scopus | 2-s2.0-78751512089 | |
| dc.identifier.uri | http://doi.org/10.1063/1.3536370 | |
| dc.identifier.uri | https://hdl.handle.net/11147/2613 | |
| dc.language.iso | en | en_US |
| dc.publisher | American Institute of Physics | en_US |
| dc.relation.ispartof | AIP Conference Proceedings | en_US |
| dc.rights | info:eu-repo/semantics/openAccess | en_US |
| dc.subject | Cataclysmic variables | en_US |
| dc.subject | Stellar evolution | en_US |
| dc.subject | Polars | en_US |
| dc.title | Magnetic Cataclysmic Variables | en_US |
| dc.type | Conference Object | en_US |
| dspace.entity.type | Publication | |
| gdc.author.institutional | Kalomeni, Belinda | |
| gdc.author.yokid | 17457 | |
| gdc.bip.impulseclass | C5 | |
| gdc.bip.influenceclass | C5 | |
| gdc.bip.popularityclass | C5 | |
| gdc.coar.access | open access | |
| gdc.coar.type | text::conference output | |
| gdc.collaboration.industrial | false | |
| gdc.description.department | İzmir Institute of Technology. Physics | en_US |
| gdc.description.endpage | 211 | en_US |
| gdc.description.publicationcategory | Konferans Öğesi - Uluslararası - Kurum Öğretim Elemanı | en_US |
| gdc.description.scopusquality | Q4 | |
| gdc.description.startpage | 210 | en_US |
| gdc.description.volume | 1314 | en_US |
| gdc.description.wosquality | N/A | |
| gdc.identifier.openalex | W2046017254 | |
| gdc.index.type | Scopus | |
| gdc.oaire.diamondjournal | false | |
| gdc.oaire.impulse | 0.0 | |
| gdc.oaire.influence | 2.635068E-9 | |
| gdc.oaire.isgreen | true | |
| gdc.oaire.keywords | Cataclysmic variables | |
| gdc.oaire.keywords | cataclysmic variables | |
| gdc.oaire.keywords | stellar evolution | |
| gdc.oaire.keywords | Polars | |
| gdc.oaire.keywords | polars | |
| gdc.oaire.keywords | Stellar evolution | |
| gdc.oaire.popularity | 5.079408E-10 | |
| gdc.oaire.publicfunded | false | |
| gdc.oaire.sciencefields | 0103 physical sciences | |
| gdc.oaire.sciencefields | 01 natural sciences | |
| gdc.openalex.collaboration | National | |
| gdc.openalex.fwci | 0.20722816 | |
| gdc.openalex.normalizedpercentile | 0.66 | |
| gdc.opencitations.count | 0 | |
| gdc.plumx.mendeley | 1 | |
| gdc.plumx.scopuscites | 0 | |
| gdc.scopus.citedcount | 0 | |
| relation.isAuthorOfPublication.latestForDiscovery | 61b0471a-1ce6-4b3b-b125-7ee8b87ac871 | |
| relation.isOrgUnitOfPublication.latestForDiscovery | 9af2b05f-28ac-4009-8abe-a4dfe192da5e |