activity
20132020
most citedA remarkable recurrent nova in M31 - The optical observations

68 citations · 217 across the 7 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2020★ 13 cited

Two New Nova Shells associated with V4362 Sagittarii and DO Aquilae

E. J. Harvey, M. P. Redman, P. Boumis +8

A classical nova is an eruption on the surface of a white dwarf in an accreting binary system. The material ejected from the white dwarf surface generally forms an axisymmetric she…

astro-ph.SR2018★ 36 cited

Breaking the habit - the peculiar 2016 eruption of the unique recurrent nova M31N 2008-12a

M. Henze, M. J. Darnley, S. C. Williams +70

Since its discovery in 2008, the Andromeda galaxy nova M31N 2008-12a has been observed in eruption every single year. This unprecedented frequency indicates an extreme object, with…

astro-ph.SR2016★ 34 cited

Deciphering the bipolar planetary nebula Abell 14 with 3D ionization and morphological studies

S. Akras, N. Clyne, P. Boumis +4

Abell 14 is a poorly studied object despite being considered a born again planetary nebula. We performed a detailed study of its 3D morphology and ionization structure using the SH…

astro-ph.SR2014★ 68 cited

A remarkable recurrent nova in M31 - The optical observations

M. J. Darnley, S. C. Williams, M. F. Bode +5

Context: In late November 2013 a fifth eruption in five years of the M31 recurrent nova M31N 2008-12a was announced. Aims: In this Letter we address the optical lightcurve and prog…

astro-ph.SR2013★ 17 cited

Rapid Dust Formation in Novae: The Speed Class - Formation Timescale Correlation Explained

S. C. Williams, M. F. Bode, M. J. Darnley +3

Observations show that the time of onset of dust formation in classical novae depends strongly on their speed class, with dust typically taking longer to form in slower novae. Usin…