Hiding in the Shadows: Searching for Planets in Pre-Transitional and Transitional Disks
dc.contributor.utaustinauthor | Dodson-Robinson, Sarah E. | en_US |
dc.creator | Dobinson, Jack | en_US |
dc.creator | Leinhardt, Zoe. M. | en_US |
dc.creator | Dodson-Robinson, Sarah E. | en_US |
dc.creator | Teanby, Nick A. | en_US |
dc.date.accessioned | 2016-10-28T19:38:45Z | |
dc.date.available | 2016-10-28T19:38:45Z | |
dc.date.issued | 2013-11 | en_US |
dc.description.abstract | Transitional and pre-transitional disks can be explained by a number of mechanisms. This work aims to find a single observationally detectable marker that would imply a planetary origin for the gap and, therefore, indirectly indicate the presence of a young planet. N-body simulations were conducted to investigate the effect of an embedded planet of one Jupiter mass on the production of instantaneous collisional dust derived from a background planetesimal disk. Our new model allows us to predict the dust distribution and resulting observable markers with greater accuracy than previous works. Dynamical influences from a planet on a circular orbit are shown to enhance dust production in the disk interior and exterior to the planet orbit, while removing planetesimals from the orbit itself, creating a clearly defined gap. In the case of an eccentric planet, the gap opened by the planet is not as clear as the circular case, but there is a detectable asymmetry in the dust disk. | en_US |
dc.description.department | Astronomy | en_US |
dc.description.sponsorship | NERC | en_US |
dc.description.sponsorship | Bristol School of Physics | en_US |
dc.description.sponsorship | McDonald Observatory | en_US |
dc.description.sponsorship | STFC | en_US |
dc.description.sponsorship | National Science Foundation AST-1055910 | en_US |
dc.description.sponsorship | Leverhulme Trust | en_US |
dc.identifier | doi:10.15781/T23B5WB31 | |
dc.identifier.citation | Dobinson, Jack, Zoë M. Leinhardt, Sarah E. Dodson-Robinson, and Nick A. Teanby. "Hiding in the Shadows: Searching for Planets in Pre-transitional and Transitional Disks." The Astrophysical Journal Letters, Vol. 777, No. 2 (Nov., 2013): L31. | en_US |
dc.identifier.doi | 10.1088/2041-8205/777/2/l31 | en_US |
dc.identifier.issn | 2041-8205 | en_US |
dc.identifier.uri | http://hdl.handle.net/2152/43129 | |
dc.language.iso | English | en_US |
dc.relation.ispartof | en_US | |
dc.relation.ispartofserial | Astrophysical Journal Letters | 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 | planet-disk interactions | en_US |
dc.subject | protoplanetary disks | en_US |
dc.subject | gm-aurigae | en_US |
dc.subject | planetesimals | en_US |
dc.subject | systems | en_US |
dc.subject | debris | en_US |
dc.subject | gas | en_US |
dc.subject | protoplanets | en_US |
dc.subject | simulation | en_US |
dc.subject | timescale | en_US |
dc.subject | signposts | en_US |
dc.subject | diversity | en_US |
dc.subject | astronomy & astrophysics | en_US |
dc.title | Hiding in the Shadows: Searching for Planets in Pre-Transitional and Transitional Disks | en_US |
dc.type | Article | en_US |