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20032018
most citedA remarkable recurrent nova in M31 - The optical observations

68 citations · 249 across the 14 of their papers we have counts for

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15 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★ 21 cited

Optical spectroscopy of Be/gamma-ray binaries

R. K. Zamanov, K. A. Stoyanov, J. Marti +4

We report optical spectroscopic observations of the Be/gamma-ray binaries LSI+61303, MWC 148 and MWC 656. The peak separation and equivalent widths of prominent emission lines (H-a…

astro-ph.SR2015★ 20 cited

Nova light curves from the Solar Mass Ejection Imager (SMEI) - II. The extended catalog

R. Hounsell, M. J. Darnley, M. F. Bode +10

We present the results from observing nine Galactic novae in eruption with the Solar Mass Ejection Imager (SMEI) between 2004 and 2009. While many of these novae reached peak magni…

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.GA2013★ 4 cited

Extragalactic Nova Populations

A. W. Shafter, C. Curtin, C. J. Pritchet +2

Nova rates have now been measured for more than a dozen galaxies spanning a wide range of Hubble types. When normalized to the infrared K-band luminosity of the galaxy, the luminos…

astro-ph.HE2011★ 2 cited

Swift observations of the March 2011 outburst of the cataclysmic variable NSV 1436: a probable dwarf nova (Research Note)

J. P. Osborne, K. L. Page, A. A. Henden +7

The March 2011 outburst of the poorly-studied cataclysmic variable NSV 1436 offered an opportunity to decide between dwarf nova and recurrent nova classifications. We use seven dai…