Add to ORKGInternational audienceIn this paper, we study the southern star-forming region located in Lupus that constitutes one of the richest associations of T Tauri stars. Based on the convergent point (CP) method combined with a k-NN analysis we identify 109 pre-main sequence stars in this region that define the Lupus association of comoving stars, and derive individual distances for all group members
IThe problem of the determination of distances has always played a central role in astronomy. Howeve...
To reliably determine the main physical parameters (masses and ages) of young stars, we must know th...
The kinematics of T Tauri stars in the nearby star forming regions Taurus-Auriga, Chamaeleon, Lupus ...
In this paper, we study the southern star-forming region located in Lupus that constitutes one of th...
International audienceIn this paper, we study the southern star-forming region located in Lupus that...
In this paper, we study the southern star-forming region located in Lupus that constitutes one of th...
In this paper, we study the southern star-forming region located in Lupus that constitutes one of th...
This paper is dedicated to investigating the kinematic properties of the Lupus moving group of young...
Aims. A precise determination of the distance to individual stars is required to reliably ...
International audienceTo reliably determine the main physical parameters (masses and ages) of young ...
To reliably determine the main physical parameters (masses and ages) of young stars, we must know th...
To reliably determine the main physical parameters (masses and ages) of young stars, we must know th...
To reliably determine the main physical parameters (masses and ages) of young stars, we must know th...
Context. Lupus is recognised as one of the closest star-forming regions, but the lack of trigonometr...
International audienceIThe problem of the determination of distances has always played a central rol...
IThe problem of the determination of distances has always played a central role in astronomy. Howeve...
To reliably determine the main physical parameters (masses and ages) of young stars, we must know th...
The kinematics of T Tauri stars in the nearby star forming regions Taurus-Auriga, Chamaeleon, Lupus ...
In this paper, we study the southern star-forming region located in Lupus that constitutes one of th...
International audienceIn this paper, we study the southern star-forming region located in Lupus that...
In this paper, we study the southern star-forming region located in Lupus that constitutes one of th...
In this paper, we study the southern star-forming region located in Lupus that constitutes one of th...
This paper is dedicated to investigating the kinematic properties of the Lupus moving group of young...
Aims. A precise determination of the distance to individual stars is required to reliably ...
International audienceTo reliably determine the main physical parameters (masses and ages) of young ...
To reliably determine the main physical parameters (masses and ages) of young stars, we must know th...
To reliably determine the main physical parameters (masses and ages) of young stars, we must know th...
To reliably determine the main physical parameters (masses and ages) of young stars, we must know th...
Context. Lupus is recognised as one of the closest star-forming regions, but the lack of trigonometr...
International audienceIThe problem of the determination of distances has always played a central rol...
IThe problem of the determination of distances has always played a central role in astronomy. Howeve...
To reliably determine the main physical parameters (masses and ages) of young stars, we must know th...
The kinematics of T Tauri stars in the nearby star forming regions Taurus-Auriga, Chamaeleon, Lupus ...