G 196-3 B or b? - Revised mass

View previous topic View next topic Go down

G 196-3 B or b? - Revised mass

Post by Edasich on 23rd September 2011, 3:38 am

Not sure whether it goes to Unconfirmed Planets thread. In that case, shift this discussion there

Do you remember G 196-3 B in Extrasolar Vision I website? Previously classed as brown dwarf companion, but according to EPE's new planetary upper limit and Zapatero Osorio et al. (2010) new mass estimate, this objects well falls witihin massive planets' domain, with mass between 12 and 25 Jupiter masses (18.5 6.5 Jupiter masses, I would say).

Paper Infrared and Kinematic Properties of the Substellar Object G 196-3 B

We report unusual near- and mid-infrared photometric properties of G 196-3 B, the young substellar companion at 16'' from the active M2.5-type star G 196-3 A, using data taken with the IRAC and MIPS instruments onboard Spitzer. G 196-3 B shows markedly redder colors at all wavelengths from 1.6 up to 24 μm than expected for its spectral type, which is determined at L3 from optical and near-infrared spectra. We discuss various physical scenarios to account for its reddish nature and conclude that a low-gravity atmosphere with enshrouded upper atmospheric layers and/or a warm dusty disk/envelope provides the most likely explanations, the two of them consistent with an age in the interval 20-300 Myr. We also present new and accurate separate proper motion measurements for G 196-3 A and B confirming that both objects are gravitationally linked and share the same motion within a few mas yr-1. After integration of the combined spectrophotometric spectral energy distributions, we obtain the result that the difference in the bolometric magnitudes of G 196-3 A and B is 6.15 0.10 mag. Kinematic consideration of the Galactic space motions of the system for distances in the interval 15-30 pc suggests that the pair is a likely member of the Local Association and that it lies near the past positions of young star clusters like α Persei less than 85 Myr ago, where the binary might have originated. At these young ages, the mass of G 196-3 B would be in the range 12-25 M Jup, close to the frontier between planets and brown dwarfs.


Emphasis mine.
avatar
Edasich
dM star
dM star

Number of posts : 1518
Location : Tau Ceti g - Mid Latitudes
Registration date : 2008-06-02

View user profile

Back to top Go down

View previous topic View next topic Back to top


 
Permissions in this forum:
You cannot reply to topics in this forum