Add to ORKGThe major characteristics in the ultraviolet of the 1982-84 eclipse of Eps Aur as observed with IUE by various workers are summarized. This star can be observed over the entire IUE wavelength range, from 1200 to 3200 A, in low dispersion, allowing eclipse light curves to be obtained in broadband regions, but due to its steep spectral gradient and the sensitivities of IUE cameras, high resolution exposures adequately cover only the regions from 1700-1900 and 2400-3200 A. In many ways, the UV data confirms or expands upon interpretations of the stem made from observations in other wavelength regions, but in other respects the system remains as enigmatic as before
Intermediate band blue (4530A), far red (7790A) and H-alpha intermediate and narrow band photoelectr...
Context. EECep is an unusual long-period (5.6 yr) eclipsing binary discovered during the mid-twentie...
Epsilon (ε) Aurigae is a binary star system that has baffled astronomers for 170 years. In 1821 it w...
The objectives were to examine, in detail, the spectra of the eclipsing binary Epsilon Aurigae taken...
The preliminary results of the study of several high resolution spectrograms (lambda 3500 - lambda 7...
Spectrophotometric scans were obtained at 8 A resolution from 3295 to 8880 A on twenty nights before...
The infrared photometry of epsilon Aur performed prior to and during the ingress phase of the recent...
It is confirmed that HR 2554 (G6 II + A0 V) is an atmospheric eclipsing system of the zeta-Aur type....
We report here on a series of medium resolution spectro-photometric observations of the enigmatic lo...
One of the major results from the IUE may prove to be the new knowledge gained by studies of the ult...
Observations of the system zeta Aurigae made around primary eclipse are described, and their signifi...
The eighteen ultraviolet light curves of Epsilon Aurigae have been plotted using the integrated flux...
We have performed spectroscopy and photometry of eclipses of the pre-cataclysmic variable UUSge usin...
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 ...
Intermediate band blue (4530A), far red (7790A) and H-alpha intermediate and narrow band photoelectr...
Context. EECep is an unusual long-period (5.6 yr) eclipsing binary discovered during the mid-twentie...
Epsilon (ε) Aurigae is a binary star system that has baffled astronomers for 170 years. In 1821 it w...
The objectives were to examine, in detail, the spectra of the eclipsing binary Epsilon Aurigae taken...
The preliminary results of the study of several high resolution spectrograms (lambda 3500 - lambda 7...
Spectrophotometric scans were obtained at 8 A resolution from 3295 to 8880 A on twenty nights before...
The infrared photometry of epsilon Aur performed prior to and during the ingress phase of the recent...
It is confirmed that HR 2554 (G6 II + A0 V) is an atmospheric eclipsing system of the zeta-Aur type....
We report here on a series of medium resolution spectro-photometric observations of the enigmatic lo...
One of the major results from the IUE may prove to be the new knowledge gained by studies of the ult...
Observations of the system zeta Aurigae made around primary eclipse are described, and their signifi...
The eighteen ultraviolet light curves of Epsilon Aurigae have been plotted using the integrated flux...
We have performed spectroscopy and photometry of eclipses of the pre-cataclysmic variable UUSge usin...
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 ...
Intermediate band blue (4530A), far red (7790A) and H-alpha intermediate and narrow band photoelectr...
Context. EECep is an unusual long-period (5.6 yr) eclipsing binary discovered during the mid-twentie...
Epsilon (ε) Aurigae is a binary star system that has baffled astronomers for 170 years. In 1821 it w...