Observations of the eclipsing dwarf nova IP Peg during outburst reveal metal lines in emission, such as Mg II 4481 Angstrom. Analysis using Doppler tomography locates emission of helium and metal lines on the inner Roche lobe of the secondary star. Such multi-line Roche-lobe imaging presents a new tool in mapping the red star's ionization structure.</p
We study the IB(s)m galaxy IC 3476 observed in the context of the Virgo Environmental Survey Tracing...
We study the IB(s)m galaxy IC 3476 observed in the context of the Virgo Environmental Survey Tracing...
An investigation of Fe II fluorescence by PAR (photoexcitation by accidental resonance) in AG Peg ha...
We analyse a unique set of time-resolved echelle spectra of the dwarf nova IP Peg, obtained at the E...
Abstract. We performed time–resolved spectroscopic studies of the double–eclipsing dwarf nova EX Dra...
We analyse a unique set of time-resolved echelle spectra of the dwarf nova IP Peg, obtained at ESO's...
Abstract. The latest outburst of AG Peg has lasted for 150 years, which makes it the slowest nova er...
We report on structure in the emissions region encountered in polars. This will become a travel alon...
Accretion is a fundamentally important process for pre-main-sequence stars, affecting disk stability...
International audienceWe present the results of our spectroscopic study of the dwarf nova SS Cyg, us...
The recurrent nova (RN) V3890 Sgr was observed during the seventh day after the onset of its most re...
The latest outburst of AG Peg has lasted for 150 years, which makes itthe slowest nova eruption ever...
STAR-MELT Python Package YouTube link to one-minute talk Accretion is a fundamentally important pr...
Debris discs which orbit white dwarfs are signatures of remnant planetary systems. We present 12 yr ...
We present high and medium resolution phase-resolved far red spectra of the magnetic cataclysmic var...
We study the IB(s)m galaxy IC 3476 observed in the context of the Virgo Environmental Survey Tracing...
We study the IB(s)m galaxy IC 3476 observed in the context of the Virgo Environmental Survey Tracing...
An investigation of Fe II fluorescence by PAR (photoexcitation by accidental resonance) in AG Peg ha...
We analyse a unique set of time-resolved echelle spectra of the dwarf nova IP Peg, obtained at the E...
Abstract. We performed time–resolved spectroscopic studies of the double–eclipsing dwarf nova EX Dra...
We analyse a unique set of time-resolved echelle spectra of the dwarf nova IP Peg, obtained at ESO's...
Abstract. The latest outburst of AG Peg has lasted for 150 years, which makes it the slowest nova er...
We report on structure in the emissions region encountered in polars. This will become a travel alon...
Accretion is a fundamentally important process for pre-main-sequence stars, affecting disk stability...
International audienceWe present the results of our spectroscopic study of the dwarf nova SS Cyg, us...
The recurrent nova (RN) V3890 Sgr was observed during the seventh day after the onset of its most re...
The latest outburst of AG Peg has lasted for 150 years, which makes itthe slowest nova eruption ever...
STAR-MELT Python Package YouTube link to one-minute talk Accretion is a fundamentally important pr...
Debris discs which orbit white dwarfs are signatures of remnant planetary systems. We present 12 yr ...
We present high and medium resolution phase-resolved far red spectra of the magnetic cataclysmic var...
We study the IB(s)m galaxy IC 3476 observed in the context of the Virgo Environmental Survey Tracing...
We study the IB(s)m galaxy IC 3476 observed in the context of the Virgo Environmental Survey Tracing...
An investigation of Fe II fluorescence by PAR (photoexcitation by accidental resonance) in AG Peg ha...