Models of Stars, Brown Dwarfs and Exoplanets
arXiv:1112.3591 · doi:10.1098/rsta.2011.0269
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.
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
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- The identification of new Herbig Ae/Be stars from LAMOST DR7
- Exoplanet host-star properties: the active environment of exoplanets
- Direct detections of white dwarfs in four WD+dM post-common envelope binaries within 20 pc
- A Catalog of Homogeneously Derived Stellar Parameters for Spectroscopic Survey Stars
- Searching for Faint Comoving Companions to the Centauri system in the VVV Survey Infrared Images
- Next-generation Exo-REM atmospheric models: application to VHS 1256 b to emulate patchy clouds
- The 2021 Hot-type Symbiotic Outburst of YY Herculis: An Optical Follow-up Study
- Dynamic Photometric Variability in Three Young Brown Dwarfs in Taurus: Detection of Optical Flares with TESS data
- Discovery and Characterization of Three New High-amplitude delta Scuti Stars from TESS Observations
- The search for IR excess in low signal to noise sources
- TOI-333b: A Neptune Desert planet around a F7V star
- Hidden Gems in TESS: sherlock finds two new rocky planets around nearby M dwarfs
- Confirmation of SRGt 062340.2-265751 as a nova-like cataclysmic variable with a possible magnetic nature
- A spatially-resolved large cavity of the J0337 protoplanetary disk in Perseus