TY - JOUR
T1 - The discovery of a very cool binary system
AU - Burningham, B.
AU - Leggett, S.K.
AU - Lucas, P.W.
AU - Pinfield, D.J.
AU - Smart, R.L.
AU - Day-Jones, A.C.
AU - Jones, H.R.A.
AU - Murray, D.N.
AU - Nickson, E.
AU - Tamura, M.
AU - Zhang, Z.
AU - Lodieu, N.
AU - Tinney, C.G.
AU - Zapatero Osorio, M.R.
N1 - The definitive version can be found at: http://www3.interscience.wiley.com/ Copyright Royal Astronomical Society
PY - 2010
Y1 - 2010
N2 - We report the discovery of a very cool d/sdL7+T7.5p common proper motion binary system, SDSS J1416+13AB, found by cross-matching the United Kingdom Infrared Telescope (UKIRT) Infrared Deep Sky Survey (UKIDSS) Large Area Survey Data Release 5 (UKIDSS LAS DR4) against the Sloan Digital Sky Survey Data Release 7. The d/sdL7 is blue in J−H and H−K and has other features suggestive of low metallicity and/or high gravity. The T7.5p displays spectral peculiarity seen before in earlier type dwarfs discovered in UKIDSS LAS DR4, and referred to as CH4-J-early peculiarity, where the CH4-J index, based on the absorption to the red side of the J-band peak, suggests an earlier spectral type than the H2O-J index, based on the blue side of the J-band peak, by ∼2 subtypes. We suggest that CH4-J-early peculiarity arises from low metallicity and/or high gravity, and speculate as to its use for classifying T dwarfs. UKIDSS and follow-up United Kingdom Infrared Telescope/Wide Field CAMera (UKIRT/WFCAM) photometry shows the T dwarf to have the bluest near-infrared colours yet seen for such an object with H−K=−1.31 ± 0.17 . Warm Spitzer IRAC photometry shows the T dwarf to have extremely red H−[4.5]= 4.86 ± 0.04 , which is the reddest yet seen for a substellar object. The lack of parallax measurement for the pair limits our ability to estimate parameters for the system. However, applying a conservative distance estimate of 5–15 pc suggests a projected separation in range 45–135 au. By comparing H−K:H−[4.5] colours of the T dwarf to spectral models, we estimate that Teff= 500 K and [M/H]∼− 0.30 , with log g∼ 5.0 . This suggests a mass of ∼30 MJupiter for the T dwarf and an age of ∼10 Gyr for the system. The primary would then be a 75 MJupiter object with log g∼ 5.5 and a relatively dust-free Teff∼ 1500 K atmosphere. Given the unusual properties of the system we caution that these estimates are uncertain. We eagerly await parallax measurements and high-resolution imaging which will constrain the parameters further. [Please see original online version for correct notation]
AB - We report the discovery of a very cool d/sdL7+T7.5p common proper motion binary system, SDSS J1416+13AB, found by cross-matching the United Kingdom Infrared Telescope (UKIRT) Infrared Deep Sky Survey (UKIDSS) Large Area Survey Data Release 5 (UKIDSS LAS DR4) against the Sloan Digital Sky Survey Data Release 7. The d/sdL7 is blue in J−H and H−K and has other features suggestive of low metallicity and/or high gravity. The T7.5p displays spectral peculiarity seen before in earlier type dwarfs discovered in UKIDSS LAS DR4, and referred to as CH4-J-early peculiarity, where the CH4-J index, based on the absorption to the red side of the J-band peak, suggests an earlier spectral type than the H2O-J index, based on the blue side of the J-band peak, by ∼2 subtypes. We suggest that CH4-J-early peculiarity arises from low metallicity and/or high gravity, and speculate as to its use for classifying T dwarfs. UKIDSS and follow-up United Kingdom Infrared Telescope/Wide Field CAMera (UKIRT/WFCAM) photometry shows the T dwarf to have the bluest near-infrared colours yet seen for such an object with H−K=−1.31 ± 0.17 . Warm Spitzer IRAC photometry shows the T dwarf to have extremely red H−[4.5]= 4.86 ± 0.04 , which is the reddest yet seen for a substellar object. The lack of parallax measurement for the pair limits our ability to estimate parameters for the system. However, applying a conservative distance estimate of 5–15 pc suggests a projected separation in range 45–135 au. By comparing H−K:H−[4.5] colours of the T dwarf to spectral models, we estimate that Teff= 500 K and [M/H]∼− 0.30 , with log g∼ 5.0 . This suggests a mass of ∼30 MJupiter for the T dwarf and an age of ∼10 Gyr for the system. The primary would then be a 75 MJupiter object with log g∼ 5.5 and a relatively dust-free Teff∼ 1500 K atmosphere. Given the unusual properties of the system we caution that these estimates are uncertain. We eagerly await parallax measurements and high-resolution imaging which will constrain the parameters further. [Please see original online version for correct notation]
UR - http://www.scopus.com/inward/record.url?scp=77953570025&partnerID=8YFLogxK
U2 - 10.1111/j.1365-2966.2010.16411.x
DO - 10.1111/j.1365-2966.2010.16411.x
M3 - Article
SN - 0035-8711
VL - 404
SP - 1952
EP - 1961
JO - Monthly Notices of the Royal Astronomical Society
JF - Monthly Notices of the Royal Astronomical Society
IS - 4
ER -