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J/A+A/452/567       Spectra of Nova Scuti 2005 N.2 (V477 Sct)    (Munari+, 2006)

BVI photometry and the spectroscopy of Nova Scuti 2005 N.2. Munari U., Siviero A., Navasardyan H., Dallaporta S. <Astron. Astrophys. 452, 567 (2006)> =2006A&A...452..567M
ADC_Keywords: Novae ; Spectroscopy Keywords: stars: novae, cataclysmic variables Abstract: Our CCD photometry of Nova Scuti 2005 N.2 (=V477 Sct) shows it to be a very fast nova, which is characterized by t2=3 and t3=6 days, affected by a E(B-V)≥1.3mag reddening, and which peaked at V∼9.8mag on ∼Oct. 12.0 UT. The nova was probably entering a dust condensation episode or brightness oscillations during the transition phase when it became unobservable for the seasonal conjunction with the Sun. Absolute spectrophotometry shows it to belong to the He/N class. The emission line width at half intensity is 2600km/s. At least five ripples are identified in the high resolution emission lines profiles at radial velocities ranging from -980 to +700km/s. The nova erupted at a large distance from the Sun and at an appreciable height above the Galactic plane, suggesting an association with the Galactic bulge (unusual for a He/N nova). The progenitor was too faint to be recorded on DSS1/2 survey plates, when setting the outburst amplitude to DeltaV≥11mag. Objects: --------------------------------------------------------- RA (2000) DE Designation(s) --------------------------------------------------------- 18 38 42.93 -12 16 15.6 NOVA Sct 2005 N.2 = V* V477 Sct --------------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file fluxlr.dat 31 1019 3500-7815Å absolute fluxed spectrum for 2005 Oct 27.7 halpha.dat 31 1019 Continuum normalized spectrum around Halpha for 2005 Oct 27.7 oi.dat 31 1019 Continuum normalized spectrum around OI/CaII for 2005 Oct 27.7
Byte-by-byte Description of file: fluxlr.dat halpha.dat oi.dat
Bytes Format Units Label Explanations
1- 16 F16.11 0.1nm Lambda Wavelength 20- 31 E12.7 10mW/m2/nm Flux Flux
Acknowledgements: Ulisse Munari, munari(at)pd.astro.it
(End) Patricia Vannier [CDS] 01-Jun-2006
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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