The 32 Ori moving group was discovered almost a decade ago and despite the fact that it represents the first northern, young (~20 Myr) stellar aggregate within 100 pc of the Sun, a comprehensive characterisation of the stellar content of the group has yet to be performed. We hereby present the first large-scale spectroscopic survey for new (predominantly low-mass K- and M-type) members of the 32 Ori moving group after combining kinematic and photometric data to select candidate members with Galactic space motion and positions in colour-magnitude space consistent with group membership. Final memberships are assigned on the basis of a combination of radial velocity, Hα emission and Li absorption diagnostics. We identify ~25 new members, there...
The latest results in the research of forming planetary systems have led several authors to compile ...
Context. The Orion complex is arguably the most studied star-forming region in the Galaxy. While sta...
We present results of a large scale, multi-epoch optical survey of the Ori OB1 association, carried ...
<p>The 32 Ori moving group was discovered almost a decade ago and despite the fact that it represent...
Nearby late-type stars are excellent targets to look for young objects in stellar associations and m...
International audienceAims. We are searching for new open clusters or moving groups in the solar nei...
We report on the discovery of newmembers of nearby young moving groups, exploiting the full power of...
We report on the discovery of new members of nearby young moving groups, exploiting the full power o...
In the past decade many kinematic groups of young stars (<100 Myr) were discovered in the solar neig...
Scorpius-Centaurus is the nearest OB association, and its hundreds of members are divided into subgr...
Young, co-evolving stars, free of the obscuring effects of their formation region, exist near the Su...
We report on the discovery of new members of nearby young moving groups, exploiting the full power o...
Context. Nearby late-type stars are excellent targets for seeking young objects in stellar associat...
We present the results of a wide-field (80’ x 80’) photometric and spectroscopic survey of the young...
We have identified five new members of the TW Hydrae association (TWA), 11 new members of the Pic m...
The latest results in the research of forming planetary systems have led several authors to compile ...
Context. The Orion complex is arguably the most studied star-forming region in the Galaxy. While sta...
We present results of a large scale, multi-epoch optical survey of the Ori OB1 association, carried ...
<p>The 32 Ori moving group was discovered almost a decade ago and despite the fact that it represent...
Nearby late-type stars are excellent targets to look for young objects in stellar associations and m...
International audienceAims. We are searching for new open clusters or moving groups in the solar nei...
We report on the discovery of newmembers of nearby young moving groups, exploiting the full power of...
We report on the discovery of new members of nearby young moving groups, exploiting the full power o...
In the past decade many kinematic groups of young stars (<100 Myr) were discovered in the solar neig...
Scorpius-Centaurus is the nearest OB association, and its hundreds of members are divided into subgr...
Young, co-evolving stars, free of the obscuring effects of their formation region, exist near the Su...
We report on the discovery of new members of nearby young moving groups, exploiting the full power o...
Context. Nearby late-type stars are excellent targets for seeking young objects in stellar associat...
We present the results of a wide-field (80’ x 80’) photometric and spectroscopic survey of the young...
We have identified five new members of the TW Hydrae association (TWA), 11 new members of the Pic m...
The latest results in the research of forming planetary systems have led several authors to compile ...
Context. The Orion complex is arguably the most studied star-forming region in the Galaxy. While sta...
We present results of a large scale, multi-epoch optical survey of the Ori OB1 association, carried ...