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J/A+A/539/A94       Mean spectrum  of CP Pup in 1996         (Bianchini+, 2012)

The old nova CP Puppis: a carbon nova and asynchronous polar? Bianchini A., Saygac T., Orio M., della Valle M., Williams R. <Astron. Astrophys. 539, A94 (2012)> =2012A&A...539A..94B
ADC_Keywords: Novae ; Spectroscopy Keywords: accretion, accretion disks - stars: magnetic field - novae: cataclysmic variables Abstract: CP Pup (Nova Pup 1942) showed outburst and quiescent characteristics indicating a very massive white dwarf, yet the standard spectroscopic dynamical analysis assuming an accretion disk yields an extremely low value for the white dwarf mass. However, some physical parameters and the accretion geometry are still poorly known. The nova was spectroscopically monitored between 1988 and 1996. We analyzed the whole data set in order to re-determine the spectroscopic period and examine its stability. We also looked for chemical anomalies in the spectrum. Description: We obtained the radial velocity curves for the hydrogen and helium lines from our last better quality 1996 run. The mean 1996 spectrum yields information on the chemical composition of the binary. We also searched the mean period using the multi-year data set. Objects: ------------------------------------------------- RA (2000) DE Designation(s) ------------------------------------------------- 08 11 46.1 -35 21 05 CP Pup = NOVA Pup 1942 ------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file sp03-96.dat 22 1893 CP Pup 1996 mean spectrum
Byte-by-byte Description of file: sp03-96.dat
Bytes Format Units Label Explanations
1- 8 F8.3 0.1nm lambda [4215/5122] Wavelength 11- 22 E12.7 cW/m2/nm Flux Flux (in ergs/s/cm2/Å)
Acknowledgements: Antonio Bianchini, antonio.bianchini(at)
(End) Patricia Vannier [CDS] 31-Jan-2012
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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