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Please use this identifier to cite or link to this item: http://hdl.handle.net/1959.3/56646
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- Title
- Early spectral evolution of Nova Sagittarii 2004 (V5114 Sagittarii)
- Author(s)
- Ederoclite, A.; Mason, E.; Della Valle, M.; Gilmozzi, R.; Williams, R. E.; Germany, L.; Saviane, I.; Matteucci, F.; Schaefer, B. E.; Walter, F.; Rudy, R. J.; Lynch, D.; Mazuk, S.; Venturini, C. C.; Puetter, R. C.; Perry, R. B.; Liller, W.; Rotter, A.
- Abstract
- We present optical and near-infrared spectral evolution of the Galactic nova V5114 Sgr (2004) during few months after the outburst. Methods. We use multi-band photometry and line intensities derived from spectroscopy to put constrains on the distance and the physical conditions of the ejecta of V5114 Sgr. The nova showed a fast decline t2 ≅ 11 days) and spectral features of Fen spectroscopic class. It reached
- Publication type
- Journal article
- Source
- Astronomy and Astrophysics, Vol. 459, no. 3 (2006), pp. 875-883
- Publication year
- 2006
- FOR Code(s)
- 0201 Astronomical and Space Sciences; 020110 Stellar Astronomy and Planetary Systems
- Keyword(s)
- Cataclysmic variables; Galactic novae; Galaxy evolution; Infrared spectroscope; Near-infrared spectral evolution; Photometry; Spectrum analysis; Stars; V5114 Sgr
- Publisher
- EDP Sciences
- ISSN
- 0004-6361
- Publisher URL
- http://dx.doi.org/10.1051/0004-6361:20065741
- Copyright
- Copyright © 2006 The European Southern Observatory (ESO). Published version of the paper reproduced here in accordance with the copyright policy of the publisher.
- Full text
- Peer reviewed
