Deep infrared imaging and spectroscopy of the nearby late M-dwarf DENIS-P J104814-395606
- Author(s)
- R. Neuhäuser, E. W. Guenther, J. Alves, N. Grosso, Ch. Leinert, Th. Ratzka, Th. Ott, M. Mugrauer, F. Comerón, A. Brandner, W. Eckart
- Abstract
We obtained deep H- and K-band images of DENIS-P J104814-395606 using
SofI and the speckle camera SHARP-I at the ESO-3.5m-NTT as well as QUIRC
at the Mauna Kea 2.2m telescope between December 2000 and June 2001. The
target was recently discovered as nearby M9-dwarf among DENIS sources
(Delfosse et al. 2001). We detect parallactic motion on our images and
determine the distance to be 4.6 +/- 0.3 pc, more precise than
previously known. From the available colors, the distance, and the
spectral type, we conclude from theoretical models that the star has a
mass of ~ 0.075 to 0.09 Msun and an age of ~ 1 to 2 Gyrs.
We also obtained H- and K-band spectra of this star with ISAAC at the
VLT. A faint companion candidate is detected 6'' NNW of the
star, which is 6.4 +/- 0.5 mag fainter in H. However, according to
another image taken several month later, the companion candidate is not
co-moving with the M9-dwarf. Instead, it is a non-moving background
object. Limits for undetected companion candidates are such that we can
exclude any stellar companions outside of ~ 0.25'' (1 AU),
any brown dwarf companions (above the deuterium burning mass limit)
outside of ~ 2'' (9 AU), and also any companion down to ~
40 M_jup with >= 0.15'' (0.7 AU) separation, all
calculated for an age of 2 Gyrs. Our observations show that direct
imaging of sub-stellar companions near the deuterium burning mass limit
in orbit around nearby ultra-cool dwarfs is possible, even with
separations that are smaller than the semi-major axis of the outermost
planet in our solar system, namely a few tens of AU.
- Organisation(s)
- Department of Astrophysics
- External organisation(s)
- Thüringer Landessternwarte Tautenburg, Universität zu Köln, European Southern Observatory (Germany), Max-Planck-Institut für extraterrestrische Physik, Max-Planck-Institut für Astronomie
- Journal
- Astronomische Nachrichten
- Volume
- 323
- Pages
- 447-452
- ISSN
- 0004-6337
- DOI
- https://doi.org/10.1002/1521-3994(200210)323:5<447::AID-ASNA447>3.0.CO;2-M
- Publication date
- 07-2002
- Keywords
- Portal url
- https://ucrisportal.univie.ac.at/en/publications/1848016f-a0bf-4941-b05c-ad3d378c2f4e