Basit öğe kaydını göster

The final decline of Nova (V1974) Cygni 1992 and discovery of an associated extended emission nebulosity

dc.contributor.authorRosino, L.
dc.contributor.authorEsenoglu, Hasan Hüseyin
dc.contributor.authorDella Valle, Massimo
dc.contributor.authorIijima, Takashi
dc.contributor.authorRafanelli, P.
dc.contributor.authorRadovich, M.
dc.date.accessioned2021-03-03T16:16:15Z
dc.date.available2021-03-03T16:16:15Z
dc.date.issued1996
dc.identifier.citationRosino L., Iijima T., Rafanelli P., Radovich M., Esenoglu H. H. , Della Valle M., "The final decline of Nova (V1974) Cygni 1992 and discovery of an associated extended emission nebulosity", ASTRONOMY & ASTROPHYSICS, cilt.315, sa.3, ss.463-466, 1996
dc.identifier.issn0004-6361
dc.identifier.othervv_1032021
dc.identifier.otherav_435ca07d-79f4-492b-98ec-45a2a9ef2735
dc.identifier.urihttp://hdl.handle.net/20.500.12627/48996
dc.description.abstractNew spectroscopic observations of Nova Cygni 1992 (V1974 Cyg) carried out in 1994-95 have shown a progressive decrease of the ionization level, made evident by the fading or disappearance of the emission lines of [Ne V], [Ne III], [Fe VII], [Fe VI] and [O III], which were outstanding in the 1992-93 spectra. An echelle spectrum obtained at Asiago in October 1995 clearly shows the complexity of the velocity field of the nova.
dc.language.isoeng
dc.subjectFizik
dc.subjectAstronomi ve Astrofizik
dc.subjectTemel Bilimler
dc.subjectTemel Bilimler (SCI)
dc.subjectUzay bilimi
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.titleThe final decline of Nova (V1974) Cygni 1992 and discovery of an associated extended emission nebulosity
dc.typeMakale
dc.relation.journalASTRONOMY & ASTROPHYSICS
dc.contributor.department, ,
dc.identifier.volume315
dc.identifier.issue3
dc.identifier.startpage463
dc.identifier.endpage466
dc.contributor.firstauthorID40524


Bu öğenin dosyaları:

DosyalarBoyutBiçimGöster

Bu öğe ile ilişkili dosya yok.

Bu öğe aşağıdaki koleksiyon(lar)da görünmektedir.

Basit öğe kaydını göster