2007A&A...464..787S


C.D.S. - SIMBAD4 rel 1.7 - 2019.11.14CET19:04:47

2007A&A...464..787S - Astronomy and Astrophysics, volume 464, 787-791 (2007/3-3)

Nearby star candidates in the Torino observatory parallax program.

SMART R.L., LATTANZI M.G., JAHREISS H., BUCCIARELLI B. and MASSONE G.

Abstract (from CDS):

Candidates with suspect distances from the Catalog of Nearby Stars were included in the Torino Observatory Parallax Program with the goal to clarify their membership in that catalog. Observations of the objects were made over the period 1996-2001 on the 1.05m Torino telescope. The trigonometric parallaxes and proper motions were determined using standard techniques. Of the 22 objects examined, 11 are within the 25pc horizon of the Catalog of Nearby Stars. The remaining objects are either misclassified, sub-dwarfs rather than main sequence dwarfs with consequently overestimated photometric distances, or objects with published trigonometric parallaxes that are incorrect.

Abstract Copyright:

Journal keyword(s): astrometry - methods: data analysis - stars: distances - stars: fundamental parameters - subdwarfs - stars: low-mass, dwarfs brown

Simbad objects: 22

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Number of rows : 22

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
#notes
1 G 32-5 PM* 00 15 49.2423890520 +13 33 22.318401892   14.0 12.600 12.296 10.04 M4V 50 0
2 GD 806 PM* 01 12 27.4113570783 -01 51 22.793997622   14.60 14.11 14.10 13.55 ~ 9 0
3 GJ 3140 LP* 02 10 13.5275664707 +11 31 59.637716863     12.72   9.85 M4III 9 0
4 EGGR 169 WD* 04 25 53.7275747770 +12 11 48.335004184   15.96 15.44 15.54 14.77 DA8 43 0
5 G 82-25 PM* 04 31 07.3273676928 -05 20 25.959512028   15.3 13.612 13.288   M3.5 14 0
6 Cl* Melotte 25 LH 27 * 04 34 59.2321815786 +17 33 38.051241277   18.28 16.38   12.55 ~ 2 0
7 G 234-53 PM* 09 02 52.8712809804 +68 03 46.573190998   14.0 12.622 12.357 9.75 M4.0Ve 23 0
8 LP 370-26 PM* 09 29 11.0784784045 +25 58 09.277079507   18.16 16.457 14.808 12.847 M5.0 20 1
9 LP 261-205 PM* 10 09 16.8674708157 +35 14 52.200574087   16.8 16.46 14.66 12.76 M5.5V 10 0
10 G 44-42 PM* 10 52 04.2435209218 +13 59 51.304932595   13.9 12.737 12.336 9.95 M4V 40 0
11 PG 1126+186 WD* 11 29 18.0379393674 +18 16 45.647483463   13.37 14.10   13.23 DC+G/K(e) 18 0
12 LP 732-35 PM* 11 31 08.3876130622 -14 57 21.250346429 16.97 15.97 14.24 14.33 10.94 M5 34 0
13 Ross 119 Fl* 11 54 07.8867656818 +09 48 22.809337399   14.47 12.852 12.596 9.92 M4.0V 36 0
14 LP 319-53 PM* 11 56 54.8695071807 +26 39 56.430933734   16.6 15.51 14.8 13.00 esdM1.0 16 0
15 LP 675-8 PM* 12 24 26.8092517525 -04 43 36.760637333   16.542 14.934 13.985 13.052 M3.0VI 16 0
16 LP 377-13 PM* 12 34 15.7823162026 +20 37 05.791313655   19.9 17.69 17.0 15.01 sdM4.5 16 0
17 G 164-47 Fl* 13 09 34.9715315862 +28 59 06.362525584   15.93 14.078 13.707 11.14 M4.8V 56 0
18 LP 269-79 PM* 13 37 17.3564997355 +35 01 01.446825865   17.2 16.37 14.2 13.00 ~ 8 0
19 LP 558-40 PM* 13 46 55.5340679502 +05 42 56.453286427   16.4 15.223 14.290 13.410 M0.0VI 15 0
20 Ross 848 PM* 14 20 07.3705760426 -09 37 13.391646267   14.47 12.87   10.25 M4 42 0
21 LP 270-67 PM* 14 20 52.9107951337 +36 57 17.230926996   17.20 16.17 14.67 12.85 M5V 15 0
22 G 156-63 PM* 22 54 46.547880 -05 28 28.46712       13.61 11.21 M4 20 0

    Equat.    Gal    SGal    Ecl

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2019.11.14-19:04:47

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