2006A&A...459..669K


C.D.S. - SIMBAD4 rel 1.7 - 2021.03.03CET03:31:48

2006A&A...459..669K - Astronomy and Astrophysics, volume 459, 669-678 (2006/11-4)

Deep imaging survey of the environment of α Centauri. I. Adaptive optics imaging of αCenB with VLT-NACO.

KERVELLA P., THEVENIN F., COUDE DU FORESTO V. and MIGNARD F.

Abstract (from CDS):

α Centauri is our closest stellar neighbor, at a distance of only 1.3pc, and its two main components have spectral types comparable to the Sun. This is therefore a favorable target for an imaging search for extrasolar planets. Moreover, indications exist that the gravitational mass of α Cen B is higher than its modeled mass, the difference being consistent with a substellar companion of a few tens of Jupiter masses. We searched for faint comoving companions to α Cen B. As a secondary objective, we built a catalogue of the detected background sources. We used the NACO adaptive optics system of the VLT in the J, H, and Ks bands to search for companions to αCenB. This instrument allowed us to achieve a very high sensitivity to point-like sources, with a limiting magnitude of mKs≃18 at 7'' from the star. We complemented this data set with archival coronagraphic images from the HST-ACS instrument to obtain an accurate astrometric calibration. Over the observed area, we did not detect any comoving companion to α Cen B down to an absolute magnitude of 19-20 in the H and Ks bands. However, we present a catalogue of 252 background objects within about 15'' of the star. This catalogue fills part of the large void area that surrounds αCen in sky surveys due to the strong diffused light. We also present a model of the diffused light as a function of angular distance for the NACO instrument, that can be used to predict the background level for bright star observations. According to recent numerical models, the limiting magnitude of our search sets the maximum mass of possible companions to 20-30 times Jupiter, between 7 and 20AU from α Cen B.

Abstract Copyright:

Journal keyword(s): techniques: high angular resolution - stars: individual: α Cen - stars: planetary systems - stars: solar neighbourhood - astronomical data bases: miscellaneous - infrared: stars

VizieR on-line data: <Available at CDS (J/A+A/459/669): table7.dat>

Nomenclature: Table 7: [KTC2006] NNN (Nos 1-252).

Status at CDS : All or part of tables of objects could be ingested in SIMBAD with priority 2.

Simbad objects: 12

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Number of rows : 12

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2021
#notes
1 V* CC Phe Ro* 01 28 08.6609551392 -52 38 19.147504694   9.98 9.07     K1V 71 1
2 * ups And PM* 01 36 47.84216 +41 24 19.6443 4.70 4.64 4.10 3.64 3.35 F9V 900 1
3 * tau Boo Ro* 13 47 15.74340 +17 27 24.8552 5.02 4.98 4.49 4.09 3.85 F7IV-V 899 1
4 NAME Proxima Centauri Er* 14 29 42.9451234609 -62 40 46.170818907 14.21 12.95 11.13 9.45 7.41 M5.5Ve 1016 0
5 * alf Cen ** 14 39 29.71993 -60 49 55.9990   0.4 -0.1     G2V+K1V 843 0
6 * alf Cen B PM* 14 39 35.06311 -60 50 15.0992 2.89 2.21 1.33     K1V 915 1
7 * alf Cen A SB* 14 39 36.49400 -60 50 02.3737 0.96 0.72 0.01     G2V 1157 0
8 GAL 000.0+00.0 gam 17 45 39.60213 -29 00 22.0000           ~ 12003 0
9 * alf Lyr dS* 18 36 56.33635 +38 47 01.2802 0.03 0.03 0.03 0.07 0.10 A0Va 2538 0
10 * 16 Cyg B PM* 19 41 51.9731830550 +50 31 03.086127222 7.07 6.86 6.20 5.76 5.42 G3V 810 1
11 HD 188753 ** 19 54 58.3717655 +41 52 17.529759   8.22 7.44 6.9   G9V 127 1
12 * gam Cep SB* 23 39 20.9015326708 +77 37 56.505477975 5.190 4.250   2.6   K1III-IVCN1 558 1

    Equat.    Gal    SGal    Ecl

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