Evolution of Binaries Towards Hmxbs and Lmxbs
| dc.contributor.author | Kalomeni, Belinda | |
| dc.contributor.author | Kalomeni, Belinda | |
| dc.contributor.other | 04.05. Department of Pyhsics | |
| dc.contributor.other | 04. Faculty of Science | |
| dc.contributor.other | 01. Izmir Institute of Technology | |
| dc.coverage.doi | 10.1063/1.3629516 | |
| dc.date.accessioned | 2017-03-06T08:05:51Z | |
| dc.date.available | 2017-03-06T08:05:51Z | |
| dc.date.issued | 2011 | |
| dc.description | Astrophysics of Neutron Stars 2010 - A Conference in Honor of M. Ali Alpar; Cesme, Izmir; Turkey; 2 August 2010 through 6 August 2010 | en_US |
| dc.description.abstract | In this study we investigate the evolution of binary systems towards low mass x-ray binaries and high mass x-ray binaries using Eggleton's binary star evolution code. © 2011 American Institute of Physics. | en_US |
| dc.identifier.citation | Kalomeni, B. (2011, August 2-6). Evolution of binaries towards HMXBs and LMXBs. Paper presented at the Conference on Astrophysics of Neutron Stars in Honor of M Ali Alpar (ASTRONS). doi:10.1063/1.3629516 | en_US |
| dc.identifier.doi | 10.1063/1.3629516 | en_US |
| dc.identifier.isbn | 9780735409392 | |
| dc.identifier.issn | 0094-243X | |
| dc.identifier.scopus | 2-s2.0-80053374566 | |
| dc.identifier.uri | http://doi.org/10.1063/1.3629516 | |
| dc.identifier.uri | http://hdl.handle.net/11147/4975 | |
| 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 | Binary systems | en_US |
| dc.subject | HMXBs | en_US |
| dc.subject | LMXBs | en_US |
| dc.subject | Stellar evolution | en_US |
| dc.title | Evolution of Binaries Towards Hmxbs and Lmxbs | en_US |
| dc.type | Conference Object | en_US |
| dspace.entity.type | Publication | |
| gdc.author.institutional | Kalomeni, Belinda | |
| 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 | 205 | en_US |
| gdc.description.publicationcategory | Konferans Öğesi - Uluslararası - Kurum Öğretim Elemanı | en_US |
| gdc.description.scopusquality | Q4 | |
| gdc.description.startpage | 204 | en_US |
| gdc.description.volume | 1379 | en_US |
| gdc.description.wosquality | N/A | |
| gdc.identifier.openalex | W2021723292 | |
| gdc.identifier.wos | WOS:000302936600041 | |
| gdc.index.type | WoS | |
| 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 | Binary systems | |
| gdc.oaire.keywords | stellar evolution | |
| gdc.oaire.keywords | HMXBs | |
| gdc.oaire.keywords | LMXBs | |
| gdc.oaire.keywords | Stellar evolution | |
| gdc.oaire.popularity | 5.5947835E-10 | |
| gdc.oaire.publicfunded | false | |
| gdc.openalex.collaboration | National | |
| gdc.openalex.fwci | 0.0 | |
| gdc.openalex.normalizedpercentile | 0.08 | |
| gdc.opencitations.count | 0 | |
| gdc.plumx.scopuscites | 0 | |
| gdc.scopus.citedcount | 0 | |
| gdc.wos.citedcount | 0 | |
| relation.isAuthorOfPublication | 61b0471a-1ce6-4b3b-b125-7ee8b87ac871 | |
| relation.isAuthorOfPublication.latestForDiscovery | 61b0471a-1ce6-4b3b-b125-7ee8b87ac871 | |
| relation.isOrgUnitOfPublication | 9af2b05f-28ac-4009-8abe-a4dfe192da5e | |
| relation.isOrgUnitOfPublication | 9af2b05f-28ac-4005-8abe-a4dfe193da5e | |
| relation.isOrgUnitOfPublication | 9af2b05f-28ac-4003-8abe-a4dfe192da5e | |
| relation.isOrgUnitOfPublication.latestForDiscovery | 9af2b05f-28ac-4009-8abe-a4dfe192da5e |