The Discovery of Y Dwarfs with WISE
Michael Cushing
University of Toledo

One of the primary science goals of the Wide-field Infrared Survey Explorer (WISE), a NASA mission that surveyed the sky at four mid-infrared wavelengths, is to identify very cold (Teff < 1000 K) brown dwarfs. With atmospheric conditions similar to that of giant planets, brown dwarfs are ideal exoplanet analogs that can be observed free from the contaminating light of host stars. The study of these cold brown dwarfs will also provide constraints on the functional form of the low-mass stellar mass function and on the lower mass limit of star formation, two critical constraints on theories of star formation. To date, we have identified roughly 150 new brown dwarfs with WISE, six of which are so cold (Teff < 500 K) that the creation of a new spectral class, dubbed 'Y', was required. I will discuss the discovery of the Y dwarfs as well as our modeling effort aimed at deriving their atmospheres parameters using the model atmospheres of Marley and Saumon.

Date:	Jeudi, 9 février 2012
Time:	11:30
Where:	Université de Montréal
	Pavillon Roger-Gaudry, local D-460
Contact:	David Lafrenière