Searching for young m dwarfs with galex

Evgenya Shkolnik, Michael C. Liu, I. Neill Reid, Trent Dupuy, Alycia J. Weinberger

Research output: Contribution to journalArticle

37 Citations (Scopus)

Abstract

The census of young moving groups in the solar neighborhood is significantly incomplete in the low-mass regime. We have developed a new selection process to find these missing members based on the Galaxy Evolution Explorer (GALEX) All-Sky Imaging Survey (AIS). For stars with spectral types ≥K5 (R-J ≥ 1.5) and younger than ̃300 Myr, we show that near-UV (NUV) and far-UV (FUV) emission is greatly enhanced above the quiescent photosphere, analogous to the enhanced X-ray emission of young low-mass stars seen by ROSAT but detectable to much larger distances with GALEX. By combining GALEX data with optical (HST Guide Star Catalog) and near-IR (2MASS) photometry, we identified an initial sample of 34 youngMdwarf candidates in a 1000 deg2 region around the ≈10 Myr TW Hydra Association (TWA). Low-resolution spectroscopy of 30 of these found 16 which had Ha in emission, which were then followed up at high resolution to search for spectroscopic evidence of youth and to measure their radial velocities. Four objects have low surface gravities, photometric distances and space motions consistent with TWA, but the non-detection of Li indicates that they may be too old to belong to this moving group. One object (M3.5, 93 ± 19 pc) appears to be the first known accreting low-mass member of the ≈15 Myr Lower Centaurus Crux OB association. Two objects exhibit all the characteristics of the known TWA members, and thus we designate them as TWA 31 (M4.2, 110 ± 11 pc) and TWA 32 (M6.3, 53 ± 5 pc). TWA 31 shows extremely broad (447 km s-1) Hα emission, making it the sixth member of TWA found to have ongoing accretion. TWA 32 is resolved into a 0."6 binary in Keck laser guide star adaptive optics imaging. Our search should be sensitive down to spectral types of at least M4-M5 in TWA and thus the small numbers of new member is puzzling. This might indicate TWA has an atypical mass function or that the presence of lithium absorption may be too restrictive a criteria for selecting young low-mass stars.

Original languageEnglish (US)
JournalAstrophysical Journal
Volume727
Issue number1
DOIs
StatePublished - Jan 20 2011
Externally publishedYes

Fingerprint

Hydra
galaxies
lithium
stars
census
laser
spectroscopy
accretion
young
gravity
astronomical catalogs
laser guide stars
solar neighborhood
photosphere
adaptive optics
radial velocity
photometry
sky

Keywords

  • Open clusters and associations: individual (TW Hydra Association)
  • Stars: kinematics and dynamics
  • Stars: low-mass
  • Stars: pre-main sequence
  • Stars: variables: T Tauri, Herbig Ae/Be
  • Ultraviolet: stars

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics
  • Nuclear and High Energy Physics

Cite this

Shkolnik, E., Liu, M. C., Reid, I. N., Dupuy, T., & Weinberger, A. J. (2011). Searching for young m dwarfs with galex. Astrophysical Journal, 727(1). https://doi.org/10.1088/0004-637X/727/1/6

Searching for young m dwarfs with galex. / Shkolnik, Evgenya; Liu, Michael C.; Reid, I. Neill; Dupuy, Trent; Weinberger, Alycia J.

In: Astrophysical Journal, Vol. 727, No. 1, 20.01.2011.

Research output: Contribution to journalArticle

Shkolnik, E, Liu, MC, Reid, IN, Dupuy, T & Weinberger, AJ 2011, 'Searching for young m dwarfs with galex', Astrophysical Journal, vol. 727, no. 1. https://doi.org/10.1088/0004-637X/727/1/6
Shkolnik, Evgenya ; Liu, Michael C. ; Reid, I. Neill ; Dupuy, Trent ; Weinberger, Alycia J. / Searching for young m dwarfs with galex. In: Astrophysical Journal. 2011 ; Vol. 727, No. 1.
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