Discovery of two nearby post-T Tauri stellar associations
arXiv:2003.11725 · doi:10.3847/1538-3881/ab6b22
Abstract
In this work we report the discovery of 2 new stellar associations in close vicinity of the Sun at roughly 180 and 150 pc. These two associations, named as u Tau assoc and e Tau assoc, were detected based on their clustering in a multi-dimensional parameter space including , , , and of Gaia. The fitting of pre-main-sequence model isochrones in their color-magnitude diagrams suggests that the two associations are of about 50 Myr old and the group members lower than 0.8 are at the stage of post-T Tauri.
arXiv comment13pages, 8 figures, 2 tables, accepted for publishing in AJ
References in corpus (40)
- Gaia Data Release 2. Summary of the contents and survey properties
- On the variation of the Initial Mass Function
- PARSEC: stellar tracks and isochrones with the PAdova and TRieste Stellar Evolution Code
- Gaia Data Release 1. Summary of the astrometric, photometric, and survey properties
- Estimating distances from parallaxes IV: Distances to 1.33 billion stars in Gaia Data Release 2
- The Dartmouth Stellar Evolution Database
- The Rockstar Phase-Space Temporal Halo Finder and the Velocity Offsets of Cluster Cores
- The Pan-STARRS1 Photometric System
- Improved parameters for extrasolar transiting planets
- BANYAN. XI. The BANYAN multivariate Bayesian algorithm to identify members of young associations within 150 pc
- The Optical to Mid-Infrared Extinction Law Based on the APOGEE, Gaia DR2, Pan-STARRS1, SDSS, APASS, 2MASS and WISE Surveys
- The Stellar Population of the Chamaeleon I Star-Forming Region
- A catalogue of young runaway Hipparcos stars within 3kpc from the Sun
- New Brown Dwarfs and an Updated Initial Mass Function in Taurus
- An Infrared/X-ray Survey for New Members of the Taurus Star-Forming Region
- Comoving stars in Gaia DR1: An abundance of very wide separation co-moving pairs
- The Stellar Membership of the Taurus Star-forming Region
- The Gould's Belt Distances Survey (GOBELINS). IV. Distance, Depth and Kinematics of the Taurus Star-Forming Region
- The VLT/NaCo large program to probe the occurrence of exoplanets and brown dwarfs at wide orbits: II- Survey description, results and performances
- 17 new very low-mass members in Taurus. The brown dwarf deficit revisited
- Gaia Data Release 1. Open cluster astrometry: performance, limitations, and future prospects
- A Survey for New Members of the Taurus Star-Forming Region with the Sloan Digital Sky Survey
- The Greater Taurus-Auriga Ecosystem I: There Is A Distributed Older Population
- A refurbished convergent point method for finding moving groups in the Hipparcos Catalogue
- A WISE Survey of Circumstellar Disks in Taurus
- New low-mass members of the Octans stellar association and an updated 30-40 Myr lithium age
- Lithium-7 surface abundance in pre-MS stars. Testing theory against clusters and binary systems
- NGC 1980 is not a foreground population of Orion: Spectroscopic survey of young stars with low extinction in Orion A
- A Survey For Planetary-mass Brown Dwarfs in the Taurus and Perseus Star-forming Regions
- Multiplicity and clustering in Taurus star-forming region. I. Unexpected ultra-wide pairs of high-order multiplicity in Taurus
- Pre-main-sequence isochrones -- III. The Cluster Collaboration isochrone server
- Pre-Main sequence Turn-On as a chronometer for young clusters: NGC346 as a benchmark
- New and Known Moving Groups And Clusters Identified in a Gaia Co-Moving Catalog
- Extended stellar systems in the solar neighborhood - III. Like ships in the night: the Coma Berenices neighbor moving group
- A survey for planetary-mass brown dwarfs in the Chamaeleon I star-forming region
- A new compact young moving group around V1062 Sco
- The Optical -- Mid-infrared Extinction Law of the l=165 Sightline in the Galactic Plane: Diversity of Extinction Law in the Diffuse Interstellar Medium
- A new method for calculating the convergent point of a moving group
- A formation scenario of young stellar groups in the region of the Scorpio Centaurus OB association
- A constraint on the formation timescale of the young open cluster NGC 2264: Lithium abundance of pre-main sequence stars
Cited by in corpus (8)
- Rotation of Low-Mass Stars in Taurus with K2
- A Census of the Taurus Star-forming Region and Neighboring Associations with Gaia
- The Tau Association: A 60 Myr-Old Coeval Group at 150 pc from the Sun
- Stellar Rotation and Structure of the Persei Complex: When Does Gyrochronology Start to Work?
- Discovery of a young stellar "snake" with two dissolving cores in the solar neighborhood
- Canis Major OB1 stellar groups contents revealed by Gaia
- Precise Ages of Field Stars From White Dwarf Companions in Gaia DR2
- Exoplanet detection and its dependence on stochastic sampling of the stellar Initial Mass Function