Chromospherically active stars in the RAVE survey. II. Young dwarfs in the solar neighborhood

Žerjal, Maruša; Zwitter, Tomaž; Matijevič, Gal; Grebel, Eva K.; Kordopatis, Georges, 1985-; Munari, Ulisse; Seabroke, George; Steinmetz, Matthias, 1966-; Wojno, Jennifer Leigh; Bienaymé, Olivier; Bland-Hawthorn, J. (Joss); Conrad, Claudia, 1983-; Freeman, Ken, 1940-; Gibson, Brad K.; Gilmore, Gerry, 1951-; Kunder, A. (Andrea); Navarro, Julio F. (Julio Fernando) ; Parker, Quentin A.; Reid, Warren A. (Warren Alfred); Siviero, Alessandro; Watson, Fred (Fred G.); Wyse, Rosemary F. G.

EA Milne Centre for Astrophysics
Solar and stellar astrophysics
2017

Journal article


Rights
© 2017. The American Astronomical Society. All rights reserved.
Abstract

A large sample of over 38,000 chromospherically active candidate solar-like stars and cooler dwarfs from the RAVE survey is addressed in this paper. An improved activity identification with respect to the previous study was introduced to build a catalog of field stars in the Solar neighborhood with an excess emission flux in the calcium infrared triplet wavelength region. The central result of this work is the calibration of the age--activity relation for the main sequence dwarfs in a range from a few 10Myr up to a few Gyr. It enabled an order of magnitude age estimation of the entire active sample. Almost 15,000 stars are shown to be younger than 1Gyr and ∼2000 younger than 100Myr. The young age of the most active stars is confirmed by their position off the main sequence in the J−K versus NUV−V diagram showing strong ultraviolet excess, mid-infrared excess in the J−K versus W1−W2 diagram and very cool temperatures (J−K>0.7). They overlap with the reference pre-main sequence RAVE stars often displaying X-ray emission. The activity level increasing with the color reveals their different nature from the solar-like stars and probably represents an underlying dynamo generating magnetic fields in cool stars. 50\% of the RAVE objects from DR5 are found in the TGAS catalog and supplemented with accurate parallaxes and proper motions by Gaia. This makes the database of a large number of young stars in a combination with RAVE's radial velocities directly useful as a tracer of the very recent large-scale star formation history in the Solar neighborhood. The data are available online in the Vizier database.

Publisher
The University of Hull
Language
English
Extent
2 MB
Identifier
hull:14125

Journal

Journal title
Astrophysical journal
Publication date
2017
Publisher
IOP Publishing
DOI
10.3847/1538-4357/835/1/61
ISSN (Print)
0004-637X
ISSN (Electronic)
1538-4357
Volume
835
Issue
1
Notes

Copy of article first published in: Astrophysical journal, 2017, v.835, issue 1.

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