{ "id": "1008.1775", "version": "v1", "published": "2010-08-10T19:11:48.000Z", "updated": "2010-08-10T19:11:48.000Z", "title": "Shocks and a Giant Planet in the Disk Orbiting BP Piscium?", "authors": [ "C. Melis", "C. Gielen", "C. H. Chen", "Joseph H. Rhee", "Inseok Song", "B. Zuckerman" ], "comment": "25 pages, 4 figures, 1 table. Accepted to ApJ", "categories": [ "astro-ph.SR" ], "abstract": "Spitzer IRS spectroscopy supports the interpretation that BP Piscium, a gas and dust enshrouded star residing at high Galactic latitude, is a first-ascent giant rather than a classical T Tauri star. Our analysis suggests that BP Piscium's spectral energy distribution can be modeled as a disk with a gap that is opened by a giant planet. Modeling the rich mid-infrared emission line spectrum indicates that the solid-state emitting grains orbiting BP Piscium are primarily composed of ~75 K crystalline, magnesium-rich olivine; ~75 K crystalline, magnesium-rich pyroxene; ~200 K amorphous, magnesium-rich pyroxene; and ~200 K annealed silica ('cristobalite'). These dust grains are all sub-micron sized. The giant planet and gap model also naturally explains the location and mineralogy of the small dust grains in the disk. Disk shocks that result from disk-planet interaction generate the highly crystalline dust which is subsequently blown out of the disk mid-plane and into the disk atmosphere.", "revisions": [ { "version": "v1", "updated": "2010-08-10T19:11:48.000Z" } ], "analyses": { "keywords": [ "disk orbiting bp piscium", "giant planet", "grains orbiting bp piscium", "mid-infrared emission line spectrum", "emitting grains orbiting bp" ], "tags": [ "journal article" ], "publication": { "doi": "10.1088/0004-637X/724/1/470", "journal": "The Astrophysical Journal", "year": 2010, "month": "Nov", "volume": 724, "number": 1, "pages": 470 }, "note": { "typesetting": "TeX", "pages": 25, "language": "en", "license": "arXiv", "status": "editable", "inspire": 865015, "adsabs": "2010ApJ...724..470M" } } }