Low-mass members of nearby young stellar moving groups from Gaia EDR3. Issue 4 (10th February 2022)

• Record Type: Journal Article
• Authors: Lee, Jinhee; Song, Inseok; Murphy, Simon J
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 511:Issue 4(2022)
• Page Start: 6179
• Page End: 6192
• Publication Date: 2022-02-10
• Subjects: (stars:) brown dwarfs -- stars: late-type -- stars: low-mass -- (Galaxy:) open clusters and associations: general -- (Galaxy:)solar neighbourhood; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/stac358
• Languages: English
• ISSNs: 0035-8711

Abstract

ABSTRACT: Gaia EDR3 offers greatly improved kinematics for nearby objects, including members of nearby young stellar moving groups (NYMGs). In this study, we aim to identify low-mass NYMG members (spectral types of M0 to mid-L) in Gaia EDR3. We calculated spatio-kinematic membership probabilities by utilizing a Bayesian membership probability calculation scheme developed in our previous study. We evaluated stellar youth primarily based on colour–magnitude diagram positions. Combining spatio-kinematic membership assessment and youth evaluation, we identified ∼2900 low-mass NYMG candidate members, including ∼700 previously claimed members. In the set of ∼2200 new candidate members, ∼550 appear to be young based on NUV brightness. Our pilot spectroscopic study with Wide Field Spectrograph (WiFeS) on the ANU 2.3-m telescope observed 78 candidates, with 79 per cent confirmed as members. Using our new member sample, we estimated an isochronal age of the β Pictoris Moving Group. The mean age (∼10 Myr), which is around half the age of recent estimates, suggests either a truly younger age of the β Pictoris Moving Group or inaccuracies in contemporary isochrones. As the main results of this study, we provide lists of newly confirmed and candidate low-mass NYMG members.