| dc.contributor.author | Esenoglu, Hasan Hüseyin | |
| dc.date.accessioned | 2021-03-03T13:34:23Z | |
| dc.date.available | 2021-03-03T13:34:23Z | |
| dc.identifier.citation | Esenoglu H. H. , "A possible detected faint shell of the classical Nova QZ Aurigae", International Conference on Classical Nova Explosions, SITGES, İspanya, 20 - 24 Mayıs 2002, cilt.637, ss.548-552 | |
| dc.identifier.other | vv_1032021 | |
| dc.identifier.other | av_34d31b45-2a7a-44b7-b760-631791ba1df3 | |
| dc.identifier.uri | http://hdl.handle.net/20.500.12627/39710 | |
| dc.description.abstract | We observed the faint shell of QZ Aur (Nova Aurigae 1964) nearly 30 years of its outburst. Despite a diameter of 0.55(+0.12)(-0,16) arcsec of the intrinsic point source of QZ Aur, a narrow-band Ha image shows that the diameter of the nova shell in 1995 was 0.86(+0.14)(-0.11) arcsec. This rather faint shell exists for a nova suggests that QZ Aur is an object worthy of further study. | |
| dc.language.iso | eng | |
| dc.subject | Temel Bilimler | |
| dc.subject | Fizik | |
| dc.subject | Astronomi ve Astrofizik | |
| dc.subject | Temel Bilimler (SCI) | |
| dc.subject | Uzay bilimi | |
| dc.subject | ASTRONOMİ VE ASTROFİZİK | |
| dc.title | A possible detected faint shell of the classical Nova QZ Aurigae | |
| dc.type | Bildiri | |
| dc.contributor.department | İstanbul Üniversitesi , Fen Fakültesi (Atama Ve Fiili Başlama Tarihi: 21.09.1988) , Astronomi Ve Uzay Bilimleri Bölümü | |
| dc.identifier.volume | 637 | |
| dc.contributor.firstauthorID | 40527 | |
