SIMBAD references

2009A&A...493L..27S - Astronomy and Astrophysics, volume 493, L27-30 (2009/1-2)

Trigonometric parallaxes of ten ultracool subdwarfs.


Abstract (from CDS):

We measure absolute trigonometric parallaxes and proper motions with respect to many background galaxies for a sample of ten ultracool subdwarfs. Observations were taken in the H-band with the OMEGA2000 camera on the 3.5 m-telescope at Calar Alto, Spain during a time period of 3.5 years. For the first time, the reduction of the astrometric measurements was carried out directly with respect to background galaxies. We obtained absolute parallaxes with mean errors ranging between 1 and 3 mas. With six completely new parallaxes we more than doubled the number of benchmark ultracool (>sdM7) subdwarfs. Six stars in the MKs vs. J-Ks diagram fit perfectly to model subdwarf sequences from M7 to L4 with [M/H] between -1.0 and -1.5, whereas 4 are consistent with a moderately low metallicity ([M/H]=-0.5) from M7 to T6. All but one of our objects have large tangential velocities between 200 and 320km/s typical of the Galactic halo population. Our results are in good agreement with recent independent measurements for three of our targets and confirm the previously measured parallax and absolute magnitude MKs of the nearest and coolest (T-type) subdwarf 2MASS 0937+29 with higher accuracy. For all targets, we also obtained infrared J,H,Ks photometry at a level of a few milli-magnitudes relative to 2MASS standards.

Abstract Copyright:

Journal keyword(s): astrometry - stars: distances - stars: kinematics - stars: low-mass, brown dwarfs - subdwarfs - solar neighborhood

VizieR on-line data: <Available at CDS (J/A+A/493/L27): table1.dat table2.dat>

CDS comments: Table 1 SDSS 1256-0224 is 2MASS J12563716-0224522 in Simbad.

Simbad objects: 11

goto Full paper

goto View the references in ADS

To bookmark this query, right click on this link: simbad:2009A&A...493L..27S and select 'bookmark this link' or equivalent in the popup menu


© Université de Strasbourg/CNRS

    • Contact