High-contrast imaging of Sirius A with VLT/SPHERE: looking for giant planets down to one astronomical unit

被引:77
作者
Vigan, A. [1 ,2 ]
Gry, C. [1 ]
Salter, G. [1 ]
Mesa, D. [3 ]
Homeier, D. [4 ,5 ]
Moutou, C. [1 ,6 ]
Allard, F. [5 ]
机构
[1] Aix Marseille Univ, CNRS, LAM, UMR 7326, F-13388 Marseille, France
[2] European So Observ, Santiago 19001, Chile
[3] Osserv Astron Padova, INAF, I-35122 Padua, Italy
[4] Heidelberg Univ, Zentrum Astron, D-69117 Heidelberg, Germany
[5] Univ Lyon, Ecole Normale Super Lyon, CRAL, UMR CNRS 5574, F-69364 Lyon 07, France
[6] Canada France Hawaii Telescope Corp, CNRS, Kamuela, HI 96743 USA
基金
欧洲研究理事会;
关键词
methods: data analysis; techniques: high angular resolution; stars: individual: Sirius A; planetary systems; LOW-MASS STARS; BROWN DWARFS; EVOLUTIONARY MODELS; EXTRASOLAR PLANETS; FAINT COMPANIONS; BINARY-SYSTEMS; T-TRANSITION; COLOR ENIGMA; ATMOSPHERES; EXOPLANETS;
D O I
10.1093/mnras/stv1928
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Sirius has always attracted a lot of scientific interest, especially after the discovery of a companion white dwarf at the end of the 19th century. Very early on, the existence of a potential third bodywas put forward to explain some of the observed properties of the system. We present new coronagraphic observations obtained with VLT/SPHERE (Very Large Telescope/SpectroPolarimetric High-contrast Exoplanet REsearch) that explore, for the very first time, the innermost regions of the system down to 0.2 arcsec(0.5 au) from Sirius A. Our observations cover the near-infrared from 0.95 to 2.3 mu m and they offer the best on-sky contrast ever reached at these angular separations. After detailing the steps of our SPHERE/IRDIFS data analysis, we present a robust method to derive detection limits for multispectral data from high-contrast imagers and spectrographs. In terms of raw performance, we report contrasts of 14.3 mag at 0.2 arcsec, similar to 16.3 mag in the 0.4-1.0 arcsec range and down to 19 mag at 3.7 arcsec. In physical units, our observations are sensitive to giant planets down to 11 M-Jup at 0.5 au, 6-7 M-Jup in the 1-2 au range and similar to 4 M-Jup at 10 au. Despite the exceptional sensitivity of our observations, we do not report the detection of additional companions around Sirius A. Using a Monte Carlo orbital analysis, we show that we can reject, with about 50 per cent probability, the existence of an 8 M-Jup planet orbiting at 1 au.
引用
收藏
页码:129 / 143
页数:15
相关论文
共 59 条
[1]   Searching for companions down to 2 AU from β Pictoris using the L'-band AGPM coronagraph on VLT/NACO [J].
Absil, O. ;
Milli, J. ;
Mawet, D. ;
Lagrange, A. -M. ;
Girard, J. ;
Chauvin, G. ;
Boccaletti, A. ;
Delacroix, C. ;
Surdej, J. .
ASTRONOMY & ASTROPHYSICS, 2013, 559
[2]   THE INFLUENCE OF H2O LINE BLANKETING ON THE SPECTRA OF COOL DWARF STARS [J].
ALLARD, F ;
HAUSCHILDT, PH ;
MILLER, S ;
TENNYSON, J .
ASTROPHYSICAL JOURNAL, 1994, 426 (01) :L39-L41
[3]   The limiting effects of dust in brown dwarf model atmospheres [J].
Allard, F ;
Hauschildt, PH ;
Alexander, DR ;
Tamanai, A ;
Schweitzer, A .
ASTROPHYSICAL JOURNAL, 2001, 556 (01) :357-372
[4]   Model atmospheres of very low mass stars and brown dwarfs [J].
Allard, F ;
Hauschildt, PH ;
Alexander, DR ;
Starrfield, S .
ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, 1997, 35 :137-177
[5]  
Allard F., 2013, MSAIS, V24, P128, DOI [10.48550/arXiv.1302.6559, DOI 10.48550/ARXIV.1302.6559]
[6]  
[Anonymous], 1960, JO
[7]   BIGRE: A LOW CROSS-TALK INTEGRAL FIELD UNIT TAILORED FOR EXTRASOLAR PLANETS IMAGING SPECTROSCOPY [J].
Antichi, Jacopo ;
Dohlen, Kjetil ;
Gratton, Raffaele G. ;
Mesa, Dino ;
Claudi, Riccardo U. ;
Giro, Enrico ;
Boccaletti, Anthony ;
Mouillet, David ;
Puget, Pascal ;
Beuzit, Jean-Luc .
ASTROPHYSICAL JOURNAL, 2009, 695 (02) :1042-1057
[8]  
Baize P., 1931, ASTRONOMIE, V45, P383
[9]   Evolutionary models for cool brown dwarfs and extrasolar giant planets. The case of HD 209458 [J].
Baraffe, I ;
Chabrier, G ;
Barman, TS ;
Allard, F ;
Hauschildt, PH .
ASTRONOMY & ASTROPHYSICS, 2003, 402 (02) :701-712
[10]   New evolutionary models for pre-main sequence and main sequence low-mass stars down to the hydrogen-burning limit [J].
Baraffe, Isabelle ;
Homeier, Derek ;
Allard, France ;
Chabrier, Gilles .
ASTRONOMY & ASTROPHYSICS, 2015, 577