Observational (IR) and optical data are presented of the newly discovered Be/X-ray binary system LSI + 61° 235, taken over the period 1991 August – 1992 May. Though the IR shows little evidence for any changes, the optical Hα spectrum has undergone substantial modification. Combination of optical photometric measurements with the IR photometry allows the overall spectrum to be investigated and the existence of the Be star’s circumstellar disc to be directly confirmed
It had been proposed earlier that the hard X-ray and gamma-ray radiation of the Be/X-ray system LSI ...
The unusual Be binary LSI +61°303 was observed by the ASCA X-ray satellite twice during the 26 day o...
Context. Be/X-ray binaries (BeXRBs) are the most populous class of high-mass X-ray binaries. Their X...
We report optical spectroscopic observations of the Be/γ-ray binaries LSI+61303, MWC 148 and MWC 656...
The Be massive X-ray binary LSI+61°303 is a 26.5 days periodic radiosource (Taylor & Gregory, 1984),...
We present new optical and infrared photometric observations and high resolution H α spectra of the ...
We present new optical and infrared photometric observations and high resolution Hα spectra of the p...
Optical and near-infrared observations are compiled for the three gamma-ray binaries hosting Be star...
This work deals with the study of Be/X-ray binaries using a multi-wavelength approach and the inform...
Context. Be/X-ray binaries represent the main group of high-mass X-ray binaries. The determination o...
Context. Current X-ray missions are regularly discovering new X/γ-ray sources, so identifying the co...
We report optical and infrared photometric and spectroscopic observations that identify the counterp...
Context. Present X-ray missions are regularly discovering new X-ray and γ-ray sources. The identific...
As displaying different transient optical and X-ray behaviors both among themselves and individually...
We present the results of a multiwavelength monitoring campaign targeting the c-ray source 2CG 135]1...
It had been proposed earlier that the hard X-ray and gamma-ray radiation of the Be/X-ray system LSI ...
The unusual Be binary LSI +61°303 was observed by the ASCA X-ray satellite twice during the 26 day o...
Context. Be/X-ray binaries (BeXRBs) are the most populous class of high-mass X-ray binaries. Their X...
We report optical spectroscopic observations of the Be/γ-ray binaries LSI+61303, MWC 148 and MWC 656...
The Be massive X-ray binary LSI+61°303 is a 26.5 days periodic radiosource (Taylor & Gregory, 1984),...
We present new optical and infrared photometric observations and high resolution H α spectra of the ...
We present new optical and infrared photometric observations and high resolution Hα spectra of the p...
Optical and near-infrared observations are compiled for the three gamma-ray binaries hosting Be star...
This work deals with the study of Be/X-ray binaries using a multi-wavelength approach and the inform...
Context. Be/X-ray binaries represent the main group of high-mass X-ray binaries. The determination o...
Context. Current X-ray missions are regularly discovering new X/γ-ray sources, so identifying the co...
We report optical and infrared photometric and spectroscopic observations that identify the counterp...
Context. Present X-ray missions are regularly discovering new X-ray and γ-ray sources. The identific...
As displaying different transient optical and X-ray behaviors both among themselves and individually...
We present the results of a multiwavelength monitoring campaign targeting the c-ray source 2CG 135]1...
It had been proposed earlier that the hard X-ray and gamma-ray radiation of the Be/X-ray system LSI ...
The unusual Be binary LSI +61°303 was observed by the ASCA X-ray satellite twice during the 26 day o...
Context. Be/X-ray binaries (BeXRBs) are the most populous class of high-mass X-ray binaries. Their X...