SIMBAD references

2000MNRAS.316..827R - Mon. Not. R. Astron. Soc., 316, 827-844 (2000/August-3)

Low-mass spectroscopic binaries in the Hyades: a candidate brown dwarf companion.

REID I.N. and MAHONEY S.

Abstract (from CDS):

We have used the HIRES echelle spectrograph on the Keck I telescope to obtain high-resolution spectroscopy of 51 late-type M dwarfs in the Hyades cluster. Cross-correlating the calibrated data against spectra of white dwarfs allows us to determine heliocentric velocities with an accuracy of ±0.3km.s–1. 27 stars were observed at two epochs in 1997; two stars, RHy 42 and RHy 403, are confirmed spectroscopic binaries. RHy 42 is a double-lined, equal-mass system; RHy 403 is a single-lined, short-period binary, P∼1.275d. RHy 403A has an absolute magnitude of MI=10.85, consistent with a mass of 0.15M. The systemic mass function has a value M2sin(i)]3/(M1+M2)2=0.0085, which, combined with the non-detection of a secondary peak in the cross-correlation function, implies 0.095>M2>0.07M, and the strong possibility that the companion is the first Hyades brown dwarf to be identified. Unfortunately, the maximum expected angular separation in the system is only ∼0.25mas. Five other low-mass Hyads are identified as possible spectroscopic binaries, based either on repeat observations or on a comparison between the observed radial velocity and the value expected for Hyades cluster members. Combined with HST imaging data, we infer a binary fraction between 23 and 30per cent. All of the stars are chromospherically active. RHy 281 was caught in mid-flare and, based on that detection, we estimate a flaring frequency of ∼2.5per cent for low-mass Hyades stars. Nine stars have rotational velocities, vsin(i), exceeding 20km.s–1, and most of the sample have detectable rotation. We examine the Hα emission characteristics of low-mass cluster members, and show that there is no evidence for a correlation with rotation.

Abstract Copyright: 2000, Royal Astronomical Society

Journal keyword(s): stars: chromospheres - stars: late-type - stars: low-mass, brown dwarfs - open clusters and associations: individual: Hyades

CDS comments: candidate brown dwarf companion is Cl* Melotte 25 REID 403B

Simbad objects: 108

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