Aims. Within a 200 pc sphere around the Sun, we search for the Hyades tidal tails in the Gaia DR2 dataset. Methods. We used a modified convergent-point method to search for stars with space velocities close to the space velocity of the Hyades cluster. Results. We find a clear indication for the existence of the Hyades tidal tails, a leading tail extending up to 170 pc from the centre of the Hyades with 292 stars (36 contaminants), and a trailing tail up to 70 pc with 237 stars (32 contaminants). A comparison with an N-body model of the cluster and its tails shows remarkably good coincidence. Five white dwarfs are found in the tails
We have used data from the UKIRT Hemisphere Survey (UHS) to search for substellar members of the Hya...
Tidal tails of stellar clusters are important laboratories for the evolution of stellar populations...
Using photometry and proper motions from Gaia Data Release 2, we detect a 50° long stream of about 7...
Aims. Within a 200 pc sphere around the Sun, we search for the Hyades tidal tails in the Gaia DR2 da...
International audienceAims. Within a 200 pc sphere around the Sun, we search for the Hyades tidal ta...
Already the first few years of the Gaia mission have brought a wealth of new insights into the veloc...
Gaia + PeTar projects combines N-body simulations with Gaia eDR3 data to robustly identify tidal tai...
Aims. Our scientific goal is to provide a 3D map of the nearest open cluster to the Sun, the Hyades,...
Aims. The Hyades cluster is an ideal target to study the dynamical evolution of a star cluster over ...
Aims. On the basis of the PPMXL catalogue we perform an all-sky census of the Hyades down ...
Aims. On the basis of the PPMXL catalogue (Röser et al. 2010, AJ, 139, 2440) we searched for white d...
Aims. We revisit the X-ray properties of the main sequence Hyades members and the relation between X...
International audienceAfter their birth a significant fraction of all stars pass through the tidal t...
The Hyades cluster is known to harbour ten so-called classical white dwarf members. Numerous studies...
We report the discovery of tidal structures around the intermediate-aged (‚àº700-800 Myr), nearby (‚...
We have used data from the UKIRT Hemisphere Survey (UHS) to search for substellar members of the Hya...
Tidal tails of stellar clusters are important laboratories for the evolution of stellar populations...
Using photometry and proper motions from Gaia Data Release 2, we detect a 50° long stream of about 7...
Aims. Within a 200 pc sphere around the Sun, we search for the Hyades tidal tails in the Gaia DR2 da...
International audienceAims. Within a 200 pc sphere around the Sun, we search for the Hyades tidal ta...
Already the first few years of the Gaia mission have brought a wealth of new insights into the veloc...
Gaia + PeTar projects combines N-body simulations with Gaia eDR3 data to robustly identify tidal tai...
Aims. Our scientific goal is to provide a 3D map of the nearest open cluster to the Sun, the Hyades,...
Aims. The Hyades cluster is an ideal target to study the dynamical evolution of a star cluster over ...
Aims. On the basis of the PPMXL catalogue we perform an all-sky census of the Hyades down ...
Aims. On the basis of the PPMXL catalogue (Röser et al. 2010, AJ, 139, 2440) we searched for white d...
Aims. We revisit the X-ray properties of the main sequence Hyades members and the relation between X...
International audienceAfter their birth a significant fraction of all stars pass through the tidal t...
The Hyades cluster is known to harbour ten so-called classical white dwarf members. Numerous studies...
We report the discovery of tidal structures around the intermediate-aged (‚àº700-800 Myr), nearby (‚...
We have used data from the UKIRT Hemisphere Survey (UHS) to search for substellar members of the Hya...
Tidal tails of stellar clusters are important laboratories for the evolution of stellar populations...
Using photometry and proper motions from Gaia Data Release 2, we detect a 50° long stream of about 7...