Add to ORKGThe preliminary results of the study of several high resolution spectrograms (lambda 3500 - lambda 7000 A), obtained at the Haute Provence Observatory (OHP) in France, at different epochs before, during and after the eclipse are reported. Some of these spectrograms are compared with corresponding IUE high resolution observations, in order to study the effects of the intrinsic UV activity, towards the longer wavelengths
It is confirmed that HR 2554 (G6 II + A0 V) is an atmospheric eclipsing system of the zeta-Aur type....
One of the major results from the IUE may prove to be the knowledge gained by studies of the ultravi...
Context. EE Cep is an unusual long-period (5.6 yr) eclipsing binary discovered during the ...
The major characteristics in the ultraviolet of the 1982-84 eclipse of Eps Aur as observed with IUE ...
Spectrophotometric scans were obtained at 8 A resolution from 3295 to 8880 A on twenty nights before...
The objectives were to examine, in detail, the spectra of the eclipsing binary Epsilon Aurigae taken...
We have performed spectroscopy and photometry of eclipses of the pre-cataclysmic variable UUSge usin...
Intermediate band blue (4530A), far red (7790A) and H-alpha intermediate and narrow band photoelectr...
The infrared photometry of epsilon Aur performed prior to and during the ingress phase of the recent...
We report here on a series of medium resolution spectro-photometric observations of the enigmatic lo...
The eighteen ultraviolet light curves of Epsilon Aurigae have been plotted using the integrated flux...
Observations of the system zeta Aurigae made around primary eclipse are described, and their signifi...
A rare eclipse of the mysterious object ε Aurigae will occur in 2009-2011. We report an updated sing...
One of the major results from the IUE may prove to be the new knowledge gained by studies of the ult...
International audienceSolar irradiance spectral measurements were performed during a total solar ecl...
It is confirmed that HR 2554 (G6 II + A0 V) is an atmospheric eclipsing system of the zeta-Aur type....
One of the major results from the IUE may prove to be the knowledge gained by studies of the ultravi...
Context. EE Cep is an unusual long-period (5.6 yr) eclipsing binary discovered during the ...
The major characteristics in the ultraviolet of the 1982-84 eclipse of Eps Aur as observed with IUE ...
Spectrophotometric scans were obtained at 8 A resolution from 3295 to 8880 A on twenty nights before...
The objectives were to examine, in detail, the spectra of the eclipsing binary Epsilon Aurigae taken...
We have performed spectroscopy and photometry of eclipses of the pre-cataclysmic variable UUSge usin...
Intermediate band blue (4530A), far red (7790A) and H-alpha intermediate and narrow band photoelectr...
The infrared photometry of epsilon Aur performed prior to and during the ingress phase of the recent...
We report here on a series of medium resolution spectro-photometric observations of the enigmatic lo...
The eighteen ultraviolet light curves of Epsilon Aurigae have been plotted using the integrated flux...
Observations of the system zeta Aurigae made around primary eclipse are described, and their signifi...
A rare eclipse of the mysterious object ε Aurigae will occur in 2009-2011. We report an updated sing...
One of the major results from the IUE may prove to be the new knowledge gained by studies of the ult...
International audienceSolar irradiance spectral measurements were performed during a total solar ecl...
It is confirmed that HR 2554 (G6 II + A0 V) is an atmospheric eclipsing system of the zeta-Aur type....
One of the major results from the IUE may prove to be the knowledge gained by studies of the ultravi...
Context. EE Cep is an unusual long-period (5.6 yr) eclipsing binary discovered during the ...