Add to ORKGV2051 Oph is an eclipsing dwarf novae with an orbital period of 90 min. This system belongs to a small group of ultrashort period eclipsing dwarf nova together with Z Cha, OY Car and HT Cas. We report a study of the spectra and structure of the accretion disc of the V2051 Oph while the star was in an unusual, faint brightness state during 1996. The analysis is based on high-speed ultraviolet and optical spectroscopy secured with the Hubble Space Telescope
We have analyzed HST archival and IUE NEWSIPS archival SWP spectra of the dwarf novae CM Del and AH ...
Time-resolved eclipse spectroscopy of the nova-like variable UXUMa obtained with the HST/FOS on 1994...
RS Ophiuchi (RS Oph) is a symbiotic variable and a recurrent nova (RN). We have monitored it with th...
We report on high-speed eclipse photometry of the dwarf nova V2051 Oph while it was in a low brightn...
We report on high-speed eclipse photometry of the dwarf nova V2051 Oph while it was in a low brightn...
We have detected coherent oscillations, at multiple frequencies, in the line and continuum emission ...
We present the results of a synthetic spectral analysis of HST STIS spectra of five long-period dwar...
The dwarf nova U Gem is unique in having a direct measurement of the K velocity of its white dwarf f...
We analyse simultaneous UBVR quiescent light curves of the cataclysmic variable V2051 Oph using the ...
We analyse simultaneous UBVR quiescent light curves of the cataclysmic variable V2051 Oph using the ...
We have re-examined two archival HST FOS G130H spectra of the prototype dwarf nova U Geminorum obtai...
Aims. The aims of our study are to improve the orbital elements of the giant and to derive the spec...
We present the results of 26 nights of CCD photometry of the nova V2540 Oph (2002) from 2003 to 2004...
We present the results of the analysis of light curves of V2051 Oph through an outburst with eclipse...
The A-type star HR 6412 = V2368 Oph was used by several investigators as a photometric comparison st...
We have analyzed HST archival and IUE NEWSIPS archival SWP spectra of the dwarf novae CM Del and AH ...
Time-resolved eclipse spectroscopy of the nova-like variable UXUMa obtained with the HST/FOS on 1994...
RS Ophiuchi (RS Oph) is a symbiotic variable and a recurrent nova (RN). We have monitored it with th...
We report on high-speed eclipse photometry of the dwarf nova V2051 Oph while it was in a low brightn...
We report on high-speed eclipse photometry of the dwarf nova V2051 Oph while it was in a low brightn...
We have detected coherent oscillations, at multiple frequencies, in the line and continuum emission ...
We present the results of a synthetic spectral analysis of HST STIS spectra of five long-period dwar...
The dwarf nova U Gem is unique in having a direct measurement of the K velocity of its white dwarf f...
We analyse simultaneous UBVR quiescent light curves of the cataclysmic variable V2051 Oph using the ...
We analyse simultaneous UBVR quiescent light curves of the cataclysmic variable V2051 Oph using the ...
We have re-examined two archival HST FOS G130H spectra of the prototype dwarf nova U Geminorum obtai...
Aims. The aims of our study are to improve the orbital elements of the giant and to derive the spec...
We present the results of 26 nights of CCD photometry of the nova V2540 Oph (2002) from 2003 to 2004...
We present the results of the analysis of light curves of V2051 Oph through an outburst with eclipse...
The A-type star HR 6412 = V2368 Oph was used by several investigators as a photometric comparison st...
We have analyzed HST archival and IUE NEWSIPS archival SWP spectra of the dwarf novae CM Del and AH ...
Time-resolved eclipse spectroscopy of the nova-like variable UXUMa obtained with the HST/FOS on 1994...
RS Ophiuchi (RS Oph) is a symbiotic variable and a recurrent nova (RN). We have monitored it with th...