New Neighbors: Parallaxes of 18 nearby stars selected from the LSPM-north catalog
arXiv:0901.3756 · doi:10.1088/0004-6256/137/5/4109
Abstract
We present astrometric parallaxes for 18 suspected nearby stars selected from the LSPM-north proper motion catalog. Sixteen objects are confirmed to be main sequence M dwarfs within 16 parsecs of the Sun, including three stars (LSPM J0011+5908, LSPM J0330+5413, LSPM J0510+2714) which lie just within the 10 parsec horizon. Two other targets (LSPM J1817+1328, LSPM J2325+1403) are confirmed to be nearby white dwarfs at distances of 14 and 22 parsecs, respectively. One of our targets, the common proper motion pair LSPM J0405+7116E + LSPM J0405+7116W, is revealed to be a triple system, with the western component resolved into a pair of 16th magnitude stars (LSPM J0405+7116W-A and LSPM J0405+7116W-B) with a 0.7"+/-0.1" angular separation. We find two stars (LSPM J1314+1320 and LSPM J1757+7042) to be significantly overluminous for their colors, and suggest that these may be unresolved doubles/multiples.
10 pages, to appear in the Astronomical Journal. Version 2, corrected for typos and small errors
References in corpus (15)
- The Solar Neighborhood XVII: Parallax Results from the CTIOPI 0.9m Program -- Twenty New Members of the RECONS 10 Parsec Sample
- Activity and Kinematics of Ultracool Dwarfs Including An Amazing Flare Observation
- New Distant Companions to Known Nearby Stars. II. Faint companions of Hipparcos stars and the frequency of wide binary systems
- Meeting the Cool Neighbors X: Ultracool dwarfs from the 2MASS All-Sky Data Release
- Spectroscopic Identification of Cool White Dwarfs in the Solar Neighbourhood
- Parallax and Luminosity Measurements of an L Subdwarf
- New High Proper Motion Stars from the Digitized Sky Survey. IV. Completion of the Southern Survey and 170 Additional Stars with pm>0.45 arcsec/yr
- Five new very low mass binaries
- The Solar Neighborhood. XIX. Discovery and Characterization of 33 New Nearby White Dwarf Systems
- Trigonometric Parallaxes for Two Late-Type Subdwarfs: LSR1425+71 (sdM8.0) and the Binary LSR1610-00 (sd?M6pec)
- Parallax and Distance Estimates for Twelve Cataclysmic Variable Stars
- The Solar Neighborhood. XVIII. Discovery of new proper motion stars with 0.40 arcsec yr^-1 > mu >= 0.18 arcsec yr^-1 between declinations -90 degrees and -47 degrees
- Optical spectroscopy of high proper motion stars: new M dwarfs within 10 pc and the closest pair of subdwarfs
- The Unusual Cataclysmic Binary Star RBS 0490 and the Space Density of Cataclysmics
- Spectroscopic distances of 28 nearby star candidates
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- CARMENES input catalogue of M dwarfs. I. Low-resolution spectroscopy with CAFOS
- CARMENES input catalogue of M dwarfs V. Luminosities, colours, and spectral energy distributions
- BANYAN. V. A Systematic All-Sky Survey for New Very Late-Type Low-Mass Stars and Brown Dwarfs in Nearby Young Moving Groups
- A Volume-Limited Sample of Ultracool Dwarfs. I. Construction, Space Density, and a Gap in the L/T Transition
- The Solar Neighborhood. XXI. Parallax Results from the CTIOPI 0.9m Program: 20 New Members of the 25 Parsec White Dwarf Sample
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- Simultaneous Multiwavelength Observations of Magnetic Activity in Ultracool Dwarfs. IV. The Active, Young Binary NLTT 33370 AB (=2MASS J13142039+1320011)
- The Volume-Complete Sample of M Dwarfs with Masses 0.1 <= M/M_sol <= 0.3 within 15 Parsecs
- The Second Arecibo Search for 5 GHz Radio Flares from Ultracool Dwarfs
- Modelling the environment around five ultracool dwarfs via the radio domain