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Pregled bibliografske jedinice broj: 415599

The nature and evolution of Nova Cygni 2006


Munari, Ulisse; Siviero, Alessandro; Henden, Arne; Cardarelli G.; Cherini, Giulio; Dallaporta, Sergio; Dalla Via, Giorgio; Frigo, Aldo; Jurdana-Šepić, Rajka; Moretti, Stefano et al.
The nature and evolution of Nova Cygni 2006 // Astronomy and Astrophysics, 492 (2008), 1; 145-166 doi:10.1051/0004-6361:200809502 (međunarodna recenzija, članak, znanstveni)


Naslov
The nature and evolution of Nova Cygni 2006

Autori
Munari, Ulisse ; Siviero, Alessandro ; Henden, Arne ; Cardarelli G. ; Cherini, Giulio ; Dallaporta, Sergio ; Dalla Via, Giorgio ; Frigo, Aldo ; Jurdana-Šepić, Rajka ; Moretti, Stefano ; Navasardyan, Hripsime ; Ochner, Paolo ; Tomaselli, Salvatore ; Tomasoni, S. ; Valisa, Paolo ; Valentini, Marica

Izvornik
Astronomy and Astrophysics (0935-4956) 492 (2008), 1; 145-166

Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni

Ključne riječi
Stars: dwarf novae ; stars: individual: V2362 Cyg

Sažetak
Nova Cyg 2006 has been intensively observed throughout its full outburst. We investigate the energetics and evolution of the central source and of the expanding ejecta, their chemical abundances and ionization structure, and the formation of dust. Methods: We recorded low, medium, and/or high-resolution spectra (calibrated into accurate absolute fluxes) on 39 nights, along with 2353 photometric UBVR_cIc measures on 313 nights, and complemented them with IR data from the literature. Results: The nova displayed initially the normal photometric and spectroscopic evolution of a fast nova of the FeII-type. Pre-maximum, principal, diffuse-enhanced, and Orion absorption systems developed in a normal way. After the initial outburst, the nova progressively slowed its fading pace until the decline reversed and a second maximum was reached (eight months later), accompanied by large spectroscopic changes. Following the rapid decline from second maximum, the nova finally entered the nebular phase and formed optically thin dust. We performed a photo-ionization analysis of the emission-line spectrum during the nebular phase, which showed a strong enrichment of the ejecta in nitrogen and oxygen, and none in neon, in agreement with theoretical predictions for the estimated 1.0 M_ȯ white dwarf in Nova Cyg 2006. The similarities with the poorly investigated V1493 Nova Aql 1999a are discussed.

Izvorni jezik
Engleski

Znanstvena područja
Fizika



POVEZANOST RADA


Projekt / tema
316-0091361-2825 - Razvoj i modeliranje fizičkih koncepata u učioničkom i e-okruženju (Rajka Jurdana-Šepić, )

Ustanove
Sveučilište u Rijeci - Odjel za fiziku

Autor s matičnim brojem:
Rajka Jurdana-Šepić, (170374)

Časopis indeksira:


  • Current Contents Connect (CCC)
  • Web of Science Core Collection (WoSCC)
    • Science Citation Index Expanded (SCI-EXP)
    • SCI-EXP, SSCI i/ili A&HCI
  • Scopus


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