| dc.contributor.author | Esenoğlu, HH | |
| dc.contributor.author | Saygac, AT | |
| dc.contributor.author | Bianchini, A | |
| dc.contributor.author | Retter, A | |
| dc.contributor.author | Özkan, M. Türker | |
| dc.contributor.author | Altan, M | |
| dc.date.accessioned | 2019-10-23T17:55:59Z | |
| dc.date.available | 2019-10-23T17:55:59Z | |
| dc.date.issued | 2000 | |
| dc.identifier.issn | 0004-6361 | |
| dc.identifier.uri | https://hdl.handle.net/11421/22790 | |
| dc.description | WOS: 000166412300026 | en_US |
| dc.description.abstract | We find an expansion parallax for the slow nova RW UMi (Nova Ursae Minoris 1956). A narrow-band H-alpha image shows that the diameter of the nova shell in 1995 was 2.94(+0.37)(-0.49) arcsec. We derive a distance of 5250(+590)(-1050) pc, and an absolute magnitude at maximum of M-v = -7.7(+0.3)(-0.4) which are consistent with previous estimates for the nova. We also revised known relations between various parameters of nova systems. | en_US |
| dc.language.iso | eng | en_US |
| dc.publisher | Edp Sciences S A | en_US |
| dc.rights | info:eu-repo/semantics/closedAccess | en_US |
| dc.subject | Stars : Distances | en_US |
| dc.subject | Stars : Individual : Nova Ursae Minoris 1956 | en_US |
| dc.subject | Stars : Individual : Rw Umi | en_US |
| dc.subject | Stars : Novae, Cataclysmic Variables | en_US |
| dc.title | A study of RW Ursae Minoris shell | en_US |
| dc.type | article | en_US |
| dc.relation.journal | Astronomy & Astrophysics | en_US |
| dc.contributor.department | Anadolu Üniversitesi, Yer ve Uzay Bilimleri Enstitüsü | en_US |
| dc.identifier.volume | 364 | en_US |
| dc.identifier.issue | 1 | en_US |
| dc.identifier.startpage | 191 | en_US |
| dc.identifier.endpage | 198 | en_US |
| dc.relation.publicationcategory | Makale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı | en_US] |
