activity
20122018
most citedM31N 2008-12a - the remarkable recurrent nova in M31: Pan-chromatic observations of the 2015 eruption

72 citations · 192 across the 6 of their papers we have counts for

collaborators

6 papers

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★ 1 cited

M31N 2008-12a - The Remarkable Recurrent Nova in M31

M. J. Darnley

M31N 2008-12a is a remarkable recurrent nova within the Andromeda Galaxy. With eleven eruptions now identified, including eight in the past eight years, the system exhibits a recur…

astro-ph.SR2016★ 72 cited

M31N 2008-12a - the remarkable recurrent nova in M31: Pan-chromatic observations of the 2015 eruption

M. J. Darnley, M. Henze, M. F. Bode +52

The Andromeda Galaxy recurrent nova M31N 2008-12a had been observed in eruption ten times, including yearly eruptions from 2008-2014. With a measured recurrence period of $P_\mathr…

astro-ph.SR2015★ 27 cited

A remarkable recurrent nova in M 31: The 2010 eruption recovered and evidence of a six-month period

M. Henze, M. J. Darnley, F. Kabashima +3

The Andromeda Galaxy recurrent nova M31N 2008-12a has been caught in eruption nine times. Six observed eruptions in the seven years from 2008 to 2014 suggested a duty cycle of ~1 y…

astro-ph.SR2014★ 33 cited

Early-phase photometry and spectroscopy of transitional Type Ia SN 2012ht: Direct constraint on the rise time

Masayuki Yamanaka, Keiichi Maeda, Miho Kawabata +15

We report photometric and spectroscopic observations of the nearby Type Ia Supernova (SN Ia) 2012ht from days to days after -band maximum. The decline rate of th…

astro-ph.HE2012★ 23 cited

Supersoft X-rays reveal a classical nova in the M 31 globular cluster Bol 126

M. Henze, W. Pietsch, F. Haberl +17

[Abridged] Classical novae (CNe) represent the main class of supersoft X-ray sources (SSSs) in the central region of our neighbouring galaxy M 31. Only three confirmed novae and th…