activity
20072023
most citedGeometrical constraints on the origin of timing signals from black holes

190 citations · 1.5k across the 48 of their papers we have counts for

collaborators

47 papers

astro-ph.HE2023★ 11 cited

On the Observability of Recurrent Nova Super-Remnants

M. W. Healy-Kalesh, M. J. Darnley, E. J. Harvey +5

The nova super-remnant (NSR) surrounding M31N 2008-12a (12a), the annually erupting recurrent nova (RN), is the only known example of this phenomenon. As this structure has grown a…

astro-ph.HE2021★ 9 cited

Nova LMC 2009a as observed with XMM-Newton, compared with other novae

Marina Orio, Andrej Dobrotka, Ciro Pinto +9

We examine four high resolution reflection grating spectrometers (RGS) spectra of the February 2009 outburst of the luminous recurrent nova LMC 2009a. They were very complex and ri…

astro-ph.SR2020★ 20 cited

A Theory for the Maximum Magnitude versus Rate of Decline (MMRD) Relation of Classical Novae

Izumi Hachisu, Hideyuki Saio, Mariko Kato +2

We propose a theory for the MMRD relation of novae, using free-free emission model light curves built on the optically thick wind theory. We calculated for va…

astro-ph.SR2019★ 16 cited

The January 2016 eruption of recurrent nova LMC 1968

N. P. M. Kuin, K. L. Page, P. Mróz +23

We present a comprehensive review of all observations of the eclipsing recurrent Nova LMC 1968 in the Large Magellanic Cloud which was previously observed in eruption in 1968, 1990…

astro-ph.HE2019★ 3 cited

Deep XMM-Newton observations of the northern disk of M31 II: Tracing the hot interstellar medium

Patrick J. Kavanagh, Manami Sasaki, Dieter Breitschwerdt +10

Aims: We use new deep XMM-Newton observations of the northern disk of M 31 to trace the hot interstellar medium (ISM) in unprecedented detail and to characterise the physical prope…

astro-ph.SR2019★ 37 cited

On a century of extragalactic novae and the rise of the rapid recurrent novae

Matthew J. Darnley, Martin Henze

Novae are the observable outcome of a transient thermonuclear runaway on the surface of an accreting white dwarf in a close binary system. Their high peak luminosity renders them v…