{ "id": "1112.3591", "version": "v1", "published": "2011-12-15T18:11:53.000Z", "updated": "2011-12-15T18:11:53.000Z", "title": "Models of Stars, Brown Dwarfs and Exoplanets", "authors": [ "France Allard", "Derek Homeier", "Bernd Freytag" ], "comment": "Refereed paper submitted to the british journal Philosophical Transactions A as an invited review to the Theo Murphy Meeting entitled \"Water in the gas phase\" held by the Kavli Royal Society in Chichely, GB, June 13-14th 2011", "doi": "10.1098/rsta.2011.0269", "categories": [ "astro-ph.SR" ], "abstract": "Within the next few years, GAIA and several instruments aiming at imag- ing extrasolar planets will see first light. In parallel, low mass planets are being searched around red dwarfs which offer more favourable conditions, both for radial velocity de- tection and transit studies, than solar-type stars. Authors of the model atmosphere code which has allowed the detection of water vapour in the atmosphere of Hot Jupiters re- view recent advancement in modelling the stellar to substellar transition. The revised solar oxygen abundances and cloud model allow for the first time to reproduce the pho- tometric and spectroscopic properties of this transition. Also presented are highlight results of a model atmosphere grid for stars, brown dwarfs and extrasolar planets.", "revisions": [ { "version": "v1", "updated": "2011-12-15T18:11:53.000Z" } ], "analyses": { "keywords": [ "brown dwarfs", "exoplanets", "revised solar oxygen abundances", "model atmosphere code", "model atmosphere grid" ], "tags": [ "review article", "journal article" ], "publication": { "journal": "Philosophical Transactions of the Royal Society of London Series A", "year": 2012, "month": "Jun", "volume": 370, "number": 1968, "pages": 2765 }, "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1081552, "adsabs": "2012RSPTA.370.2765A" } } }