2001PASP..113..703O


Query : 2001PASP..113..703O

2001PASP..113..703O - Publ. Astron. Soc. Pac., 113, 703-714 (2001/June-0)

A spectrophotometric technique for detecting companions of low-mass M dwarfs.

OETIKER B., DURIC N., McGRAW J.T. and McGRATH M.A.

Abstract (from CDS):

The most common stars in the Galaxy are the main-sequence M dwarfs, yet current techniques are not optimized for detecting companions around the lowest mass M dwarfs, those with spectral designations ranging from M6 to M10. Described in this paper is a search for companions around such stars using a newly designed differential spectrophotometric technique. This novel method combines the strengths of the photometric and spectroscopic techniques, while it minimizes their inherent limitations. The scientific goal of this project is to search for short-period systems containing brown dwarfs and giant planets. The detection of or placing limits on such systems will help discriminate among competing theories of planetary formation.

Abstract Copyright: ∼

Journal keyword(s): planetary systems: formation - Stars: Late-Type - Stars: Low-Mass, Brown Dwarfs - Techniques: Photometric

CDS comments: Table 2: star NN 1549-29 not identified.

Simbad objects: 21

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Number of rows : 21
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 HD 18445 SB* 02 57 13.1880251976 -24 58 30.414869580   9.01 7.86     K2V 115 0
2 BD-04 782 SB* 04 15 09.5344264586 -04 25 06.381142715 11.755 10.561 9.332 8.591 7.953 K5V 62 0
3 HD 283750 BY* 04 36 48.2421502608 +27 07 55.888214520   9.19 8.10 7.4   K2.5Ve 289 0
4 HD 42581B BD* 06 10 34.80 -21 52 00.0           T6.5 549 0
5 G 51-15 PM* 08 29 49.3527921926 +26 46 33.624143059   16.87   14.736   M6.5Ve 326 0
6 BD+44 2051B PM* 11 05 30.8855820790 +43 31 17.885197587   16.45 14.45 13.4   M6.0V 279 0
7 * ksi UMa B SB* 11 18 10.8360115405 +31 31 44.821690914   5.41 4.77 4.4   G2V 345 1
8 Wolf 424 ** 12 33 17.361480 +09 01 15.79224 15.398 14.313 12.467 10.937 8.988 M5.5V 329 0
9 HD 110833 SB* 12 44 14.5460629801 +51 45 33.393759952   7.97 7.01 6.4   K3 174 0
10 HD 112758 ** 12 59 01.5612841731 -09 50 02.679322421 8.737 8.384 7.588 7.163 6.729 G9V 196 1
11 LP 271-25 LM* 14 28 43.2275214164 +33 10 39.259309081   21.2   17.8   M9Ve 262 0
12 HD 140913 SB* 15 45 07.4491027968 +28 28 11.738768232   8.664 8.053     G0V 114 0
13 V* CM Dra BY* 16 34 20.3302660573 +57 09 44.368918696   14.50 12.87 10.85 9.26 M4.5V 467 0
14 VB 8 LM* 16 55 35.2557374336 -08 23 40.753073075   18.7 16.916 14.566 12.24 M7Ve 457 0
15 HD 160202 Be* 17 40 01.0407184728 -32 12 03.838222548 6.30 6.79 6.75     B5Ve 58 0
16 NAME Barnard's star BY* 17 57 48.4984700685 +04 41 36.113879676 12.497 11.24 9.511 8.298 6.741 M4V 907 2
17 G 208-45 LM* 19 53 55.1405033909 +44 24 54.147256052   15.97 13.99 14.3 10.27 M6V 205 0
18 HD 209458 V* 22 03 10.7727465312 +18 53 03.549393384   8.21 7.63     F9V 1193 1
19 HD 239960B Er* 22 27 59.7956021455 +57 41 49.746752678           M4V 181 0
20 BD-15 6290 BY* 22 53 16.7325836486 -14 15 49.304052185 12.928 11.749 10.192 9.013 7.462 M3.5V 1106 1
21 HD 217580 SB* 23 01 51.5363732448 -03 50 55.402732729 9.199 8.428 7.464 6.934 6.482 K3V 109 0

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