Hyades tidal tails revealed by Gaia DR2

Within a 200 pc sphere around the Sun, we search for the Hyades tidal tails in the <i>Gaia<i/> DR2 dataset.<i>Methods<i/>. We used a modified convergent-point method to search for stars with space velocities close to the space velocity of the Hyades cluster.<i>Results&l...

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Bibliographic Details
Main Authors: Röser, Siegfried (Author) , Schilbach, Elena (Author) , Goldman, Bertrand (Author)
Format: Article (Journal) Editorial
Language:English
Published: 04 January 2019
In: Astronomy and astrophysics
Year: 2019, Volume: 621
ISSN:1432-0746
DOI:10.1051/0004-6361/201834608
Online Access:Verlag, Volltext: http://dx.doi.org/10.1051/0004-6361/201834608
Verlag, Volltext: https:/articles/aa/abs/2019/01/aa34608-18/aa34608-18.html
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Author Notes:Siegfried Röser, Elena Schilbach, and Bertrand Goldman
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Summary:Within a 200 pc sphere around the Sun, we search for the Hyades tidal tails in the <i>Gaia<i/> DR2 dataset.<i>Methods<i/>. We used a modified convergent-point method to search for stars with space velocities close to the space velocity of the Hyades cluster.<i>Results<i/>. 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.
Item Description:Gesehen am 16.10.2020
Physical Description:Online Resource
ISSN:1432-0746
DOI:10.1051/0004-6361/201834608