| dc.contributor.author | Robb, R.M. | |
| dc.contributor.author | Vincent, J. | |
| dc.contributor.author | Henderson, H. | |
| dc.contributor.author | Greimel, R. | |
| dc.contributor.author | Drew, J.E. | |
| dc.contributor.author | Gonzalez-Solares, E. | |
| dc.date.accessioned | 2008-12-08T15:59:28Z | |
| dc.date.available | 2008-12-08T15:59:28Z | |
| dc.date.issued | 2008 | |
| dc.identifier.citation | Robb , R M , Vincent , J , Henderson , H , Greimel , R , Drew , J E & Gonzalez-Solares , E 2008 , ' The New Contact Binary GSC 2414-0797 ' , Information Bulletin on Variable Stars , vol. 5852 . | |
| dc.identifier.issn | 1587-2440 | |
| dc.identifier.other | PURE: 148917 | |
| dc.identifier.other | PURE UUID: a080fb34-ce87-4bba-a84c-33657e80b289 | |
| dc.identifier.other | dspace: 2299/2677 | |
| dc.identifier.other | Scopus: 56349169349 | |
| dc.identifier.uri | http://hdl.handle.net/2299/2677 | |
| dc.description | Original article can be found at: http://www.konkoly.hu/ibvs/ | |
| dc.description.abstract | GSC 2414-0797 has a contact binary star type light curve, a 0.4 magnitude brightness variation with a period 0.3406 days. | en |
| dc.language.iso | eng | |
| dc.relation.ispartof | Information Bulletin on Variable Stars | |
| dc.title | The New Contact Binary GSC 2414-0797 | en |
| dc.contributor.institution | School of Physics, Astronomy and Mathematics | |
| dc.contributor.institution | Science & Technology Research Institute | |
| dc.contributor.institution | Centre for Astrophysics Research | |
| dc.description.status | Peer reviewed | |
| rioxxterms.type | Journal Article/Review | |
| herts.preservation.rarelyaccessed | true | |
