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20102026
most citedLong-term eclipse timing of white dwarf binaries: an observational hint of a magnetic mechanism at work

58 citations · 155 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2026★ 2 cited

Extreme mass loss during common envelope evolution: the origin of the double low-mass white dwarf system J2102--4145

Leandro G. Althaus, Alejandro H. Corsico, Monica Zorotovic +3

Eclipsing close double white dwarf (WD) systems provide a unique opportunity to directly constrain hydrogen-envelope retention and test common-envelope (CE) evolution in low-mass s…

astro-ph.SR2021★ 13 cited

Orbital and atmospheric parameters of two wide O-type subdwarf binaries: BD11162 and Feige 80

Francisco Molina, Joris Vos, Péter Németh +4

There are 23 long-period binary systems discovered to date that contain a B-type hot subdwarf(sdB) whose orbital parameters have been fully solved. They evolve into O-type subdwarf…

astro-ph.SR2020★ 23 cited

The luminosity evolution of nova shells -- I. A new analysis of old data

C. Tappert, N. Vogt, A. Ederoclite +3

We present a re-analysis of the H and [OIII] flux data from the only comprehensive study of the luminosity evolution of nova shells, undertaken almost two decades ago. We use ne…

astro-ph.SR2017★ 4 cited

Photometric long-term variations and superhump occurrence in the Classical Nova RR Pictoris

I. Fuentes-Morales, N. Vogt, C. Tappert +3

We present an analysis of all available time-resolved photometry from the literature and new light curves obtained in 2013-2014 for the old nova RR Pictoris. The well-known hump li…

astro-ph.SR2016★ 58 cited

Long-term eclipse timing of white dwarf binaries: an observational hint of a magnetic mechanism at work

M. C. P. Bours, T. R. Marsh, S. G. Parsons +18

We present a long-term programme for timing the eclipses of white dwarfs in close binaries to measure apparent and/or real variations in their orbital periods. Our programme includ…

astro-ph.SR2010★ 55 cited

Periodic mass loss episodes due to an oscillation mode with variable amplitude in the hot supergiant HD50064

C. Aerts, K. Lefever, A. Baglin +15

We aim to interpret the photometric and spectroscopic variability of the luminous blue variable supergiant HD\,50064 ().CoRoT space photometry and follow-up high-resolution…