2009AJ....137.4109L


Query : 2009AJ....137.4109L

2009AJ....137.4109L - Astron. J., 137, 4109-4117 (2009/May-0)

New neighbors: parallaxes of 18 nearby stars selected from the LSPM-north catalog.

LEPINE S., THORSTENSEN J.R., SHARA M.M. and RICH R.M.

Abstract (from CDS):

We present astrometric parallaxes for 18 suspected nearby stars selected from the LSPM-north proper motion catalog. 16 objects are confirmed to be main-sequence M dwarfs within 16 pc of the Sun, including three stars (LSPM J0011+5908, LSPM J0330+5413, and LSPM J0510+2714) which lie just within the 10 pc horizon. Two other targets (LSPM J1817+1328, LSPM J2325+1403) are confirmed to be nearby white dwarfs at distances of 14 and 22 pc, 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 conclude that these may be unresolved doubles/multiples.

Abstract Copyright: ∼

Journal keyword(s): astrometry - binaries: visual - stars: distances - stars: low-mass, brown dwarfs - solar neighborhood - white dwarfs

Simbad objects: 23

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Number of rows : 23
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 GAT 1367 PM* 00 11 31.8200796716 +59 08 39.884054670   16.7 15.68 14.9 12.01 M6.0V 45 0
2 LSPM J0330+5413 PM* 03 30 48.8903332104 +54 13 55.155593784   17.3 15.96 14.9 12.06 M7V 30 0
3 NAME Perseus Cloud SFR 03 35.0 +31 13           ~ 1553 0
4 1RXS J033609.2+311853 PM* 03 36 08.7018479472 +31 18 39.516789096   15.655 13.995 13.741 11.14 M4.5V 44 0
5 LP 31-302 ** 04 05 56.695920 +71 16 36.72228   16.8 16.03 15.42 12.65 dM6.0 13 0
6 G 221-27 PM* 04 05 57.5193968149 +71 16 40.778867331       13.64 11.14 dM4.5 20 0
7 LP 415-302 PM* 04 39 31.6219906599 +16 15 42.955193461   17.8 15.74 14.4 12.14 M5.5Ve 30 0
8 LSR J0510+2713 PM* 05 10 20.0874119218 +27 14 01.864442913       16.7 13.39 M7V 33 0
9 LSR J0515+5911 PM* 05 15 30.9490924521 +59 11 17.439727037   20.0 18.11 16.6 13.70 M7.0V 24 0
10 LP 206-11 ** 07 11 11.518536 +43 29 56.66532   16.7 15.90 15.746 11.92 M5.5V 44 0
11 LP 169-22 PM* 11 19 30.6103695398 +46 41 43.134707939   17.4 15.86 15.0 12.08 M5.5 31 0
12 BD+25 2534 HS* 12 37 23.5161671712 +25 03 59.867922240 9.117 10.26 10.59 10.642 10.809 sdB1(k) 268 0
13 BD+18 2647 HS* 12 41 51.7899961800 +17 31 19.750566756 10.261 11.70 11.63 11.969 12.159 sdOpec 185 1
14 LP 497-33 ** 13 14 20.376648 +13 20 01.00608   16.8 15.83 14.9 11.94 M6.0V 84 0
15 LP 500-35 PM* 14 28 04.1555758336 +13 56 13.329031046   20.1 17.65 16.2 13.35 M7V 37 0
16 LP 44-162 LM* 17 57 15.4028425766 +70 42 01.191850031   20.4 18.79 17.0 14.12 M7.5V 43 0
17 LSR J1817+1328 WD* 18 17 06.4969710720 +13 28 24.991658238   16.6 15.85 15.4 14.92 DA10 36 0
18 LP 630-81 PM* 18 26 16.5527131561 +01 46 20.983735419   17.2 14.94 14.4 11.67 M4V 16 0
19 LP 335-12 LM* 18 39 33.0748216080 +29 52 16.492032768   18.9 18.21 16.8 13.60 M6.5Ve 27 0
20 LP 44-334 ** 18 40 02.39544 +72 40 54.4404   19.0 17.62 16.1 13.25 M7.0V 19 0
21 G 185-23 PM* 19 26 01.6243505784 +24 26 17.117782944   16.2 14.300 13.877 11.19 M4.5V 29 0
22 Feige 110 HS* 23 19 58.3996844256 -05 09 56.171142864 10.360 11.45 11.50 11.970 12.145 sdO8VIIIHe5 673 1
23 LP 522-46 WD* 23 25 19.8723998499 +14 03 39.604529500   16.3 16.05 15.3 15.10 DA 37 0

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