| dc.contributor.author | OZKAN, MT | |
| dc.contributor.author | ESENOGLU, Hasan Hüseyin | |
| dc.contributor.author | Retter, A | |
| dc.contributor.author | ALTAN, M | |
| dc.contributor.author | Saygac, Ahmet Talat | |
| dc.contributor.author | Bianchini, A | |
| dc.date.accessioned | 2021-03-03T14:42:07Z | |
| dc.date.available | 2021-03-03T14:42:07Z | |
| dc.date.issued | 2000 | |
| dc.identifier.citation | ESENOGLU H. H. , Saygac A. T. , Bianchini A., Retter A., OZKAN M., ALTAN M., "A study of RW Ursae Minoris shell", ASTRONOMY & ASTROPHYSICS, cilt.364, sa.1, ss.191-198, 2000 | |
| dc.identifier.issn | 0004-6361 | |
| dc.identifier.other | vv_1032021 | |
| dc.identifier.other | av_3b009f05-e10e-451a-aba6-7d531e0f37b9 | |
| dc.identifier.uri | http://hdl.handle.net/20.500.12627/43629 | |
| 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. | |
| dc.language.iso | eng | |
| dc.subject | Fizik | |
| dc.subject | Astronomi ve Astrofizik | |
| dc.subject | Temel Bilimler | |
| dc.subject | Temel Bilimler (SCI) | |
| dc.subject | Uzay bilimi | |
| dc.subject | ASTRONOMİ VE ASTROFİZİK | |
| dc.title | A study of RW Ursae Minoris shell | |
| dc.type | Makale | |
| dc.relation.journal | ASTRONOMY & ASTROPHYSICS | |
| dc.contributor.department | , , | |
| dc.identifier.volume | 364 | |
| dc.identifier.issue | 1 | |
| dc.identifier.startpage | 191 | |
| dc.identifier.endpage | 198 | |
| dc.contributor.firstauthorID | 20815 | |
