Searching for new young stars in the Northern hemisphere: the Pisces Moving Group

Using the kinematically unbiased technique described in Binks, Jeffries & Maxted (2015), we present optical spectra for a further 122 rapidly rotating (rotation periods <6  d), X-ray active FGK stars, selected from the SuperWASP survey. We identify 17 new examples of young, probably single st...

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Bibliographic Details
Main Authors: Binks, Alex S. (Author) , Jeffries, Robin D. (Author) , Ward, Jacob L. (Author)
Format: Article (Journal)
Language:English
Published: 2018
In: Monthly notices of the Royal Astronomical Society
Year: 2017, Volume: 473, Issue: 2, Pages: 2465-2485
ISSN:1365-2966
DOI:10.1093/mnras/stx2252
Online Access:Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1093/mnras/stx2252
Verlag, kostenfrei, Volltext: https://academic.oup.com/mnras/article/473/2/2465/4110296
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Author Notes:A.S. Binks, R.D. Jeffries and J.L. Ward
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Summary:Using the kinematically unbiased technique described in Binks, Jeffries & Maxted (2015), we present optical spectra for a further 122 rapidly rotating (rotation periods <6  d), X-ray active FGK stars, selected from the SuperWASP survey. We identify 17 new examples of young, probably single stars with ages of <200 Myr and provide additional evidence for a new Northern hemisphere kinematic association: the Pisces moving group (MG). The group consists of 14 lithium-rich G- and K-type stars that have a dispersion of only ∼3 km s−1 in each Galactic space velocity coordinate. The group members are approximately coeval in the colour-magnitude diagram, with an age of 30-50 Myr, and have similar, though not identical, kinematics to the Octans-Near MG.
Item Description:Advance access publication 2017 September 9
Gesehen am 13.01.2021
Physical Description:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/stx2252