Volume 533, September 2011
|Number of page(s)||12|
|Section||Stellar structure and evolution|
|Published online||16 September 2011|
Ruling out unresolved binaries in five transitional disks
VLT/NACO deep 2.12 and 1.75 μm narrow-band imaging
RSSD, European Space Agency (ESTEC), PO Box 299
2 Herschel Science Centre, European Space Agency (ESAC), PO Box 78, 28691 Villanueva de la Cañada, Madrid, Spain
3 Gemini Observatory, c/o AURA, Casilla 603, La Serena, Chile
4 CAB (INTA-CSIC), LAEFF, PO Box 78, 28691 Villanueva de la Cañada, Madrid, Spain
5 Département de Physique and Observatoire du Mont Mégantic, Université de Montréal, C.P. 6128, Succ. Centre-Ville, Montréal, QC H3C 3J7, Canada
6 UJF-Grenoble 1/CNRS-INSU, Institut de Planétologie et d’Astrophysique de Grenoble (IPAG) UMR 5274, 38041 Grenoble, France
7 Leiden Observatory, Leiden University, PO Box 9513, 2300 RA Leiden, The Netherlands
8 Max Planck Institute for Astronomy, Königstuhl 17, 69117 Heidelberg, Germany
Accepted: 4 June 2011
Context. The presence of unresolved binaries on sub-arsecond scales could explain the existence of optically thin inner holes or gaps in circumstellar disks, which are commonly referred to as “transitional” or “cold” disks, and it is the first scenario to check before making any other assumptions.
Aims. We aim at detecting the presence of companions inside the inner hole/gap region of a sample of five well known transitional disks using spatially-resolved imaging in the near-IR with the VLT/NACO/S13 camera, which probes projected distances from the primary of typically 0.1 to 7 arcsec. The sample includes the stars DoAr 21, HD 135344B (SAO 206462), HR 4796A, T Cha, and TW Hya, spanning ages of less than 1 to 10 Myr, spectral types of A0 to K7, and hole/gap outer radii of 4 to 100 AU.
Methods. In order to enhance the contrast and to avoid saturation at the core of the point-spread function (PSF), we use narrow-band filters at 1.75 and 2.12 μm. The “locally optimized combination of images” (LOCI) algorithm is applied for an optimal speckle noise removal and PSF subtraction, providing an increase of 0.5–1.5 mag in contrast over the classic method.
Results. With the proviso that we could have missed companions owing to unfavorable projections, the VLT/NACO observations rule out the presence of unresolved companions down to an inner radius of about 01 from the primary in all five transitional disks and with a detection limit of 2 to 5 mag in contrast. In the disk outer regions the detection limits typically reach 8 to 9 mag in contrast and 4.7 mag for T Cha. Hence, the NACO images resolve part of the inner hole/gap region of all disks with the exception of TW Hya, for which the inner hole is only 4 AU. The 5σ sensitivity profiles, together with a selected evolutionary model, allow to discard stellar companions within the inner hole/gap region of T Cha, and down to the substellar regime for HD 135344B and HR 4796A. DoAr 21 is the only object from the sample of five disks for which the NACO images are sensitive enough for a detection of objects less massive than ~13 MJup that is, potential giant planets or low-mass brown dwarfs at radii larger than ~76 AU (063).
Conclusions. These new VLT/NACO observations further constrain the origin of the inner opacity cavities to be owing to closer or lower-mass companions or other mechanisms such as giant planet formation, efficient grain growth, and photoevaporation (for DoAr 21 and HR 4796A).
Key words: protoplanetary disks / planetary systems / circumstellar matter / stars: general / instrumentation: adaptive optics / stars: imaging
© ESO, 2011
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