We present a comprehensive investigation of the Ε Chamaeleontis association (Ε Cha), one of several young moving groups spread across the southern sky. We re-assess the putative membership of Ε Cha using the best available proper motion and spectrosco
Context. The nearby young stellar association ϵ Cha has an estimated age of 3–5 Myr, makin...
ABSTRACT We identify a group of ∼20 comoving, mostly southern hemisphere, ∼200 Myr old stars near Ea...
Aims. We are searching for new open clusters or moving groups in the solar neighbourhood. Methods. W...
In the past decade many kinematic groups of young stars (<100 Myr) were discovered in the solar neig...
Context. The study of the motion of the members of a given open cluster or stellar associa...
Received; accepted Context. The study of the motion of the members of a given open cluster or stella...
We present an analysis of the newly identified μTau Association (MUTA) of young stars at ≈150 pc fro...
The latest Gaia data releases (EDR3 and, soon, DR3) have greatly facilitated the identification and ...
Utilizing Hipparcos parallaxes, original radial velocities and recent literature values, new Ca ii H...
The deep southern sky surrounding the Chamaeleon dark clouds is abundant with pre-main sequence star...
Astronomy and Astrophysics 549 (2013): A15 reproduced with permission from Astronomy and Astrophysic...
Context. The star-forming regions in Chamaeleon (Cha) are among the nearest (distance ~165...
Nearby Young Moving Groups (NYMGs), i.e., loose groups of stars of age \u3c100 Myr in the solar vici...
Context. The star-forming regions in Chamaeleon (Cha) are one of the nearest (distance ~ ...
Context. The Vela-Puppis region is known to host the Vela OB2 association as well as several young c...
Context. The nearby young stellar association ϵ Cha has an estimated age of 3–5 Myr, makin...
ABSTRACT We identify a group of ∼20 comoving, mostly southern hemisphere, ∼200 Myr old stars near Ea...
Aims. We are searching for new open clusters or moving groups in the solar neighbourhood. Methods. W...
In the past decade many kinematic groups of young stars (<100 Myr) were discovered in the solar neig...
Context. The study of the motion of the members of a given open cluster or stellar associa...
Received; accepted Context. The study of the motion of the members of a given open cluster or stella...
We present an analysis of the newly identified μTau Association (MUTA) of young stars at ≈150 pc fro...
The latest Gaia data releases (EDR3 and, soon, DR3) have greatly facilitated the identification and ...
Utilizing Hipparcos parallaxes, original radial velocities and recent literature values, new Ca ii H...
The deep southern sky surrounding the Chamaeleon dark clouds is abundant with pre-main sequence star...
Astronomy and Astrophysics 549 (2013): A15 reproduced with permission from Astronomy and Astrophysic...
Context. The star-forming regions in Chamaeleon (Cha) are among the nearest (distance ~165...
Nearby Young Moving Groups (NYMGs), i.e., loose groups of stars of age \u3c100 Myr in the solar vici...
Context. The star-forming regions in Chamaeleon (Cha) are one of the nearest (distance ~ ...
Context. The Vela-Puppis region is known to host the Vela OB2 association as well as several young c...
Context. The nearby young stellar association ϵ Cha has an estimated age of 3–5 Myr, makin...
ABSTRACT We identify a group of ∼20 comoving, mostly southern hemisphere, ∼200 Myr old stars near Ea...
Aims. We are searching for new open clusters or moving groups in the solar neighbourhood. Methods. W...