Forward and back: kinematics of the Palomar 5 tidal tails

Forward and back: kinematics of the Palomar 5 tidal tails

The tidal tails of Palomar 5 (Pal 5) have been the focus of many spectroscopic studies in an attempt to identify individual stars lying along the stream and characterize their kinematics. The well-studied trailing tail has been explored out to a distance of 15- from the cluster centre, while less th...

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Bibliographic Details
Main Authors: Bernard, E.J (Author), Ferguson, A.M.N (Author), Irwin, M.J (Author), Kuzma, P.B (Author), Peñarrubia, J. (Author), Tolstoy, E. (Author), Varri, A.L (Author), Zucker, D.B (Author)
Format: Article
Language:English
Published: Oxford University Press 2022
Subjects:
Cluster centers
globular clusters: general
globular clusters: individual: Palomar 5
Globular clusters: individual: palomar 5
Globular clusters:general
Kinematics
Line strength
Measurements of
Photometric data
Probabilistics approach
Spectroscopic analysis
Spectroscopic studies
Star kinematics and dynamics
Stars
Stars abundances
stars: abundances
stars: kinematics and dynamics
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