A Wide Companion Near the Deuterium Mass Limit
ING web news release
23rd March, 2008
A team of Spanish astronomers has identified a stellar companion near the deuterium-burning mass limit located at a very wide distance,
or 670 astronomical units, from the brown dwarf UScoCTIO 108 in the very young Upper Scorpius association.
Although other substellar pairs with similar mass ratio are known, the system UScoCTIO 108A and B is the widest identified so far and possibly
has a lower gravitational bound energy than any other known low-mass binary.
It seems very difficult to explain the in situ formation of this object in a
disk by core accretion or disk instability. Given the typical size and density profile of stellar disks, there does not seem to be enough mass at such a
wide separation to form a companion of this mass, unless it has originated at a lower distance and migrated to its present location. Because of the low
binding energy, it is unlikely that the system has been ejected from a higher-mass unstable multiple system.
A more plausible scenario is that the system was originated from the disruption of a more massive core in a way similar to how other binary stars are
supposed to be formed. If the formation of these wide and very low mass systems in the denser central part of clusters is relatively frequent, this could
explain the existence of isolated planetary-mass objects as planetary-mass companions that became unbound from their primaries.
Optical and near-infrared photometry and spectroscopy using ISIS and Aux Camera on the William Herschel Telescope, among other instruments, confirmed the cool nature of both UScoCTIO 108A and B, with spectral types of M7
and M9.5, and that they are bona fide members of the Upper Scorpius association, showing low gravity and features of youth. Their inferred masses are
60±20 and 14+2-8 Jupiter masses respectively.
Composite-color IZK image of UScoCTIO 108A and B (I=blue, Z=green, K'=red). IZ images are from the AUX camera on the William Herschel Telescope,
and the image is from NICS on the Telescopio Nazionale Galileo (extracted from Béjar et al., 2008). [ JPEG ].
- V. J. S. Béjar, M. R. Zapatero Osorio, A. Pérez-Garrido, C. Alvarez, E. L. Martín, R. Rebolo, I. Villó-Pérez, and
A. Díaz-Sánchez, 2008, "Discovery of a Wide Companion near the Deuterium-burning Mass Limit in the Upper Scorpius Association", ApJ, 673, L185
- "Una extraña pareja en la constelación del Escorpión", IAC press release, 30th January, 2008.