We mainly concentrate on the analysis of the high resolution observations of V1974 Cyg (about 140 spectra), which cover 200 days and 330 days of its post-outburst evolution in the SWP and LWP cameras, respectively, at a resolution of about 25km/s. The tables contain, in a sequence, the IUE camera and image number, the date of the observation, and the measured radial velocities in km/s. The laboratory vacuum wavelengths of the transitions considered are indicated. The labels "p" and "d" refer, respectively, to the principal and the diffuse-enhanced absorption systems. Blanks mean that no reliable radial velocity measurements could be obtained.

Lamers, H.J.G.L.M., Rossi, C., Altamore, A., GONZALES RIESTRA, R., Cassatella, A. (2004). V1974 Cyg IUE spectroscopy, 420, 571.

V1974 Cyg IUE spectroscopy

ALTAMORE, Aldo;
2004-01-01

Abstract

We mainly concentrate on the analysis of the high resolution observations of V1974 Cyg (about 140 spectra), which cover 200 days and 330 days of its post-outburst evolution in the SWP and LWP cameras, respectively, at a resolution of about 25km/s. The tables contain, in a sequence, the IUE camera and image number, the date of the observation, and the measured radial velocities in km/s. The laboratory vacuum wavelengths of the transitions considered are indicated. The labels "p" and "d" refer, respectively, to the principal and the diffuse-enhanced absorption systems. Blanks mean that no reliable radial velocity measurements could be obtained.
2004
Lamers, H.J.G.L.M., Rossi, C., Altamore, A., GONZALES RIESTRA, R., Cassatella, A. (2004). V1974 Cyg IUE spectroscopy, 420, 571.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11590/269626
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