Evidence for ablated flows in the shell of the nova DQ Herculis

High-resolution long-slit Hα spectra of the shell of the old nova DQ Herculis have been obtained with the William Herschel Telescope using the ISIS spectrograph. An equatorial expansion velocity of 370 ± 14 km s−1 is derived from the spectra which, in conjunction with a narrow-band Hα image of the r...

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Bibliographic Details
Published in:Monthly notices of the Royal Astronomical Society 2007-09, Vol.380 (1), p.175-180
Main Authors: Vaytet, N. M. H., O'Brien, T. J., Rushton, A. P.
Format: Article
Language:English
Subjects:
Astronomy
Astrophysics
cataclysmic variables
Earth, ocean, space
Exact sciences and technology
novae
novae, cataclysmic variables
outflows
Spectrum analysis
Stars & galaxies
stars: individual: DQ Herculis
stars: winds
stars: winds, outflows
Supernovae
Velocity
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Summary:High-resolution long-slit Hα spectra of the shell of the old nova DQ Herculis have been obtained with the William Herschel Telescope using the ISIS spectrograph. An equatorial expansion velocity of 370 ± 14 km s−1 is derived from the spectra which, in conjunction with a narrow-band Hα image of the remnant, allows a distance estimate of 525 ± 28 pc. An equatorial ring which exhibits enhanced [N ii] emission has also been detected and the inclination angle of the shell is found to be with respect to the line of sight. The spectra also reveal tails extending from the clumps in the shell, which have a radial velocity increasing along their length. This suggests the presence of a stellar wind, collimated in the polar direction, which ablates fragments of material from the clumps and accelerates them into its stream up to a terminal velocity of the order of 800–900 km s−1.
ISSN:0035-8711
1365-2966
DOI:10.1111/j.1365-2966.2007.12057.x