23 citations · 52 across the 6 of their papers we have counts for
6 papers
Determination of the superoutburst cycle lengths of 206 SU UMa type dwarf novae
N. Vogt, E. C. Puebla, A. Contreras-Quijada
SU UMa stars are characterized by "superoutbursts" which are brighter at maximum light and which last much longer than the more frequent "ordinary" outbursts of these dwarf novae.…
Life after eruption VIII: The orbital periods of novae
I. Fuentes-Morales, C. Tappert, M. Zorotovic +5
The impact of nova eruptions on the long-term evolution of Cataclysmic Variables(CVs) is one of the least understood and intensively discussed topics in the field. Acrucial ingredi…
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…
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…
Life after eruption - V. Spectroscopy of eight candidate old novae with Gemini-South
C. Tappert, N. Vogt, L. Schmidtobreick +1
We present the analysis of photometric and spectroscopic data on eight candidates for post-nova systems. Five post-novae, V528 Aql, HS Sge, BS Sgr, GR Sgr and V999 Sgr, are success…
FH Leonis, the first dwarf nova member of a multiple star system?
N. Vogt
Sudden brightenings of HD 96273 or BD+07 2411B were observed with the HIPPARCOS satellite in 1992,which still require a convincing explanation. A new analysis of all known data of…