A Second Giant Planet In 3:2 Mean-Motion Resonance In The HD 204313 System
dc.contributor.utaustinauthor | Robertson, Paul | en_US |
dc.contributor.utaustinauthor | Endl, Michael | en_US |
dc.contributor.utaustinauthor | Cochran, William D. | en_US |
dc.contributor.utaustinauthor | MacQueen, Phillip J. | en_US |
dc.contributor.utaustinauthor | Brugamyer, Erik J. | en_US |
dc.contributor.utaustinauthor | Barnes, Stuart I. | en_US |
dc.contributor.utaustinauthor | Caldwell, Caroline | en_US |
dc.creator | Robertson, Paul | en_US |
dc.creator | Horner, Jonathan | en_US |
dc.creator | Wittenmyer, Robert A. | en_US |
dc.creator | Endl, Michael | en_US |
dc.creator | Cochran, William D. | en_US |
dc.creator | MacQueen, Phillip J. | en_US |
dc.creator | Brugamyer, Erik J. | en_US |
dc.creator | Simon, Attila E. | en_US |
dc.creator | Barnes, Stuart I. | en_US |
dc.creator | Caldwell, Caroline | en_US |
dc.date.accessioned | 2016-04-28T19:32:19Z | |
dc.date.available | 2016-04-28T19:32:19Z | |
dc.date.issued | 2012-07 | en |
dc.description.abstract | We present eight years of high-precision radial velocity (RV) data for HD 204313 from the 2.7 m Harlan J. Smith Telescope at McDonald Observatory. The star is known to have a giant planet (M sin i = 3.5 M-J) on a similar to 1900 day orbit, and a Neptune-mass planet at 0.2 AU. Using our own data in combination with the published CORALIE RVs of Segransan et al., we discover an outer Jovian (M sin i = 1.6 M-J) planet with P similar to 2800 days. Our orbital fit suggests that the planets are in a 3: 2 mean motion resonance, which would potentially affect their stability. We perform a detailed stability analysis and verify that the planets must be in resonance. | en_US |
dc.description.department | Astronomy | en_US |
dc.description.sponsorship | Australian government through ARC DP0774000 | en_US |
dc.description.sponsorship | UNSW | en_US |
dc.description.sponsorship | National Aeronautics and Space Administration NNX07AL70G, NNX09AB30G | en_US |
dc.description.sponsorship | Hungarian OTKA K76816, K83790, MB08C 81013 | en_US |
dc.description.sponsorship | Hungarian Academy of Science | en_US |
dc.identifier | doi:10.15781/T2K803 | |
dc.identifier.Filename | 2012_07_secondgiant.pdf | en_US |
dc.identifier.citation | Robertson, Paul, J. Horner, Robert A. Wittenmyer, Michael Endl, William D. Cochran, Phillip J. MacQueen, Erik J. Brugamyer, Attila E. Simon, Stuart I. Barnes, and Caroline Caldwell. "A second giant planet in 3: 2 mean-motion resonance in the HD 204313 system." The Astrophysical Journal, Vol. 754, No. 1 (Jul., 2012): 50. | en_US |
dc.identifier.doi | 10.1088/0004-637x/754/1/50 | en_US |
dc.identifier.issn | 0004-637X | en_US |
dc.identifier.uri | http://hdl.handle.net/2152/34675 | |
dc.language.iso | English | en_US |
dc.relation.ispartof | en_US | |
dc.relation.ispartofserial | Astrophysical Journal | en_US |
dc.rights | Administrative deposit of works to Texas ScholarWorks: This works author(s) is or was a University faculty member, student or staff member; this article is already available through open access or the publisher allows a PDF version of the article to be freely posted online. The library makes the deposit as a matter of fair use (for scholarly, educational, and research purposes), and to preserve the work and further secure public access to the works of the University. | en_US |
dc.rights.restriction | Open | en_US |
dc.subject | planetary systems | en_US |
dc.subject | planets and satellites: dynamical evolution and | en_US |
dc.subject | stability | en_US |
dc.subject | stars: individual (hd 204313) | en_US |
dc.subject | techniques: radial velocities | en_US |
dc.subject | solar-system | en_US |
dc.subject | timing variations | en_US |
dc.subject | trojan asteroids | en_US |
dc.subject | search program | en_US |
dc.subject | long-period | en_US |
dc.subject | low-mass | en_US |
dc.subject | stars | en_US |
dc.subject | jupiters | en_US |
dc.subject | spectrometer | en_US |
dc.subject | stability | en_US |
dc.subject | astronomy & astrophysics | en_US |
dc.title | A Second Giant Planet In 3:2 Mean-Motion Resonance In The HD 204313 System | en_US |
dc.type | Article | en_US |