TY - JOUR
T1 - Qatar-2
T2 - A K Dwarf Orbited by a Transiting Hot Jupiter and a More Massive Companion in an Outer Orbit
AU - Bryan, M.L.
AU - Alsubai, K.A.
AU - Parley, N.R.
AU - Latham, D.W.
AU - Quinn, S.N.
AU - Carter, J.A.
AU - Benjamin, B.J.
AU - Berlind, P.
AU - Brown, W.R.
AU - Jørgensen, Uffe Gråe
AU - Buchhave, Lars C. Astrup
PY - 2012/5/1
Y1 - 2012/5/1
N2 - We report the discovery and initial characterization of Qatar-2b, a hot Jupiter transiting a V = 13.3mag K dwarf in a circular orbit with a short period, P b = 1.34 days. The mass and radius of Qatar-2b are M P = 2.49 M J and R P = 1.14 R J, respectively. Radial-velocity monitoring of Qatar-2 over a span of 153 days revealed the presence of a second companion in an outer orbit. The Systemic Console yielded plausible orbits for the outer companion, with periods on the order of a year and a companion mass of at least several M J. Thus, Qatar-2 joins the short but growing list of systems with a transiting hot Jupiter and an outer companion with a much longer period. This system architecture is in sharp contrast to that found by Kepler for multi-transiting systems, which are dominated by objects smaller than Neptune, usually with tightly spaced orbits that must be nearly coplanar.
AB - We report the discovery and initial characterization of Qatar-2b, a hot Jupiter transiting a V = 13.3mag K dwarf in a circular orbit with a short period, P b = 1.34 days. The mass and radius of Qatar-2b are M P = 2.49 M J and R P = 1.14 R J, respectively. Radial-velocity monitoring of Qatar-2 over a span of 153 days revealed the presence of a second companion in an outer orbit. The Systemic Console yielded plausible orbits for the outer companion, with periods on the order of a year and a companion mass of at least several M J. Thus, Qatar-2 joins the short but growing list of systems with a transiting hot Jupiter and an outer companion with a much longer period. This system architecture is in sharp contrast to that found by Kepler for multi-transiting systems, which are dominated by objects smaller than Neptune, usually with tightly spaced orbits that must be nearly coplanar.
U2 - 10.1088/0004-637X/750/1/84
DO - 10.1088/0004-637X/750/1/84
M3 - Journal article
SN - 0004-637X
VL - 750
SP - 84
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 1
ER -