Bibcode
Sahman, D. I.; Dhillon, V. S.; Littlefair, S. P.; Hallinan, G.
Referencia bibliográfica
Monthly Notices of the Royal Astronomical Society, Volume 477, Issue 4, p.4483-4490
Fecha de publicación:
7
2018
Número de citas
10
Número de citas referidas
9
Descripción
Following our tentative discovery of a faint shell around V1315 Aql
reported in Sahman et al., we undertook deep Hα imaging and
intermediate-resolution spectroscopy of the shell. We find that the
shell has its geometric centre located on V1315 Aql. The mass, spectral
features, and density of the shell are consistent with other nova
shells, rather than planetary nebulae or supernova remnants. The radial
velocity of the shell is consistent with the systemic velocity of V1315
Aql. We believe this evidence strongly suggests that the shell
originates from an earlier nova event. This is the first nova shell
discovered around a nova-like and supports the theory of nova-induced
cycles in mass transfer rates (hibernation theory) first proposed by
Shara et al.
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