From radial velocities derived from optical spectroscopic observations performed at CTIO, Chile, and CASLEO. Argentina, we have discovered that LSS 1135 is a single-lined O-type binary system with an orbital period of 2.7532 days. We present an analysis of the orbital elements of this system based on radial velocities of the He absorption lines. We classify the spectrum of LSS 1135 as O6.5V((f)). We also present spectral classifications and radial velocities for other seven OB stars in the region of Bochum 7, an OB association to which LSS 1135 belongs. Our data indicate a distance of 5.0 kpc for this star group.Facultad de Ciencias Astronómicas y Geofísica
We announce the discovery of a new early-type, double-lined spectroscopic binary in the LH 54 OB ass...
We present the results of a radial-velocity study of eight Am stars (HD 341, 55822, 61250, 67317, 93...
A new high-quality set of orbital parameters for the O-type spectroscopic binary HD 93205 has been o...
From radial velocities derived from optical spectroscopic observations performed at CTIO, Chile, and...
From radial velocities derived from optical spectroscopic observations performed at CTIO, Chile, and...
The 'All Sky Automated Survey' (ASAS) photometric observations of LS 1135, an O-type single-lined bi...
The lack of tightly bound and easily identifiable young open clusters leads to the quest for OB asso...
Context. The presence of a Wolf-Rayet star, WR12, at α = 8h44m47.2s , δ = −45◦58 55.5 (J2000.0), tri...
Aims. We plan to identify the members of the Bochum 7 association by performing simultaneous astrome...
Context. The presence of a Wolf-Rayet star, WR12, at α = 8 h44m47.2s, δ = -45°58′55. 5″ (J2000.0), t...
We present a new V light curve of the early type Magellanic eclipsing binary Sk-67°105, based on cha...
Context.The presence of a Wolf-Rayet star, WR12, at $\alpha =\rm 8^h44^m47.2^s$, $\delta = - 45^{\c...
Accepted Received; in original form Using photometric and spectroscopic observations of the double-l...
From radial velocities determined in high signal-to-noise digital spectra, we report the discovery t...
Using photometric and spectroscopic observations of the double-lined early-type eclipsingbinary syst...
We announce the discovery of a new early-type, double-lined spectroscopic binary in the LH 54 OB ass...
We present the results of a radial-velocity study of eight Am stars (HD 341, 55822, 61250, 67317, 93...
A new high-quality set of orbital parameters for the O-type spectroscopic binary HD 93205 has been o...
From radial velocities derived from optical spectroscopic observations performed at CTIO, Chile, and...
From radial velocities derived from optical spectroscopic observations performed at CTIO, Chile, and...
The 'All Sky Automated Survey' (ASAS) photometric observations of LS 1135, an O-type single-lined bi...
The lack of tightly bound and easily identifiable young open clusters leads to the quest for OB asso...
Context. The presence of a Wolf-Rayet star, WR12, at α = 8h44m47.2s , δ = −45◦58 55.5 (J2000.0), tri...
Aims. We plan to identify the members of the Bochum 7 association by performing simultaneous astrome...
Context. The presence of a Wolf-Rayet star, WR12, at α = 8 h44m47.2s, δ = -45°58′55. 5″ (J2000.0), t...
We present a new V light curve of the early type Magellanic eclipsing binary Sk-67°105, based on cha...
Context.The presence of a Wolf-Rayet star, WR12, at $\alpha =\rm 8^h44^m47.2^s$, $\delta = - 45^{\c...
Accepted Received; in original form Using photometric and spectroscopic observations of the double-l...
From radial velocities determined in high signal-to-noise digital spectra, we report the discovery t...
Using photometric and spectroscopic observations of the double-lined early-type eclipsingbinary syst...
We announce the discovery of a new early-type, double-lined spectroscopic binary in the LH 54 OB ass...
We present the results of a radial-velocity study of eight Am stars (HD 341, 55822, 61250, 67317, 93...
A new high-quality set of orbital parameters for the O-type spectroscopic binary HD 93205 has been o...