2MASS J03105986+1648155AB - A new binary at the L/T transition
arXiv:1003.3807 · doi:10.1051/0004-6361/200913711
Abstract
The transition from the L to the T spectral type of brown dwarfs is marked by a very rapid transition phase, remarkable brightening in the J-band and a higher binary frequency. Despite being an active area of inquiry, this transition regime still remains one of the most poorly understood phases of brown dwarf evolution. We resolved the L dwarf 2MASS J03105986+1648155 for the first time into two almost equally bright components straddling the L/T transition. Since such a co-eval system with common age and composition provides crucial information of this special transition phase, we monitored the system over 3 years to derive first orbital parameters and dynamical mass estimates, as well as a spectral type determination. We obtained resolved high angular resolution, near-IR images with HST and the adaptive optics instrument NACO at the VLT including the laser guide star system PARSEC. Based on two epochs of astrometric data we derive a minimum semi-major axis of 5.2 +- 0.8 AU. The assumption of a face-on circular orbit yields an orbital period of 72 +- 4 years and a total system mass of 30-60 Mjup. This places the masses of the individual components of the system at the lower end of the mass regime of brown dwarfs. The achieved photometry allowed a first spectral type determination of L9 +- 1 for each component. In addition, this seems to be only the fifth resolved L/T transition binary with a flux reversal. While ultimate explanations for this effect are still owing, the 2MASS J03105986+1648155 system adds an important benchmark object for improving our understanding of this remarkable evolutionary phase of brown dwarfs. Additionally, the observational results of 2MASS J03105986+1648155 AB derived with the new PARSEC AO system at the VLT show the importance of this technical capability. The updated AO system allows us to significantly extend the sample of brown dwarfs observable with high-resolution from the ground and hence to reveal more of their physical properties.
6 pages, 2 figures, 3 tables, accepted for publication by A&A
References in corpus (4)
- The Evolution of L and T Dwarfs in Color-Magnitude Diagrams
- Hubble Space Telescope NICMOS Observations of T Dwarfs: Brown Dwarf Multiplicity and New Probes of the L/T Transition
- Discovery of a T Dwarf Binary with the Largest Known J-Band Flux Reversal
- Discovery of a nearby L-T transition object in the Southern Galactic plane
Cited by in corpus (12)
- A Patchy Cloud Model for the L to T Dwarf Transition
- Brown Dwarf Photospheres are Patchy: A Hubble Space Telescope Near-infrared Spectroscopic Survey Finds Frequent Low-level Variability
- SpeX Spectroscopy of Unresolved Very Low Mass Binaries. II. Identification of Fourteen Candidate Binaries with Late-M/Early-L and T Dwarf Components
- Photometry and Proper Motions of M, L, and T Dwarfs from the Pan-STARRS1 3 Survey
- Discovery of a Highly Unequal-Mass Binary T Dwarf with Keck Laser Guide Star Adaptive Optics: A Coevality Test of Substellar Theoretical Models and Effective Temperatures
- NPARSEC: NTT Parallaxes of Southern Extremely Cool objects. Goals, targets, procedures and first results
- WISE2150-7520AB: A very low mass, wide co-moving brown dwarf system discovered through the citizen science project Backyard Worlds: Planet 9
- Discovery of two L & T binaries with wide separations and peculiar photometric properties
- Redder than Red: Discovery of an Exceptionally Red L/T Transition Dwarf
- On the Correlation between L Dwarf Optical and Infrared Variability and Radio Aurorae
- The search for planetary mass companions to field brown dwarfs with HST/NICMOS
- Resolving the L/T transition binary SDSS J2052-1609 AB