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Four Decades of IRC +10216: Evolution of a Carbon Rich Dust Shell Resolved at 10 microns with MMT Adaptive Optics and MIRAC4
Jared R. Males, Laird M. Close, Andrew J. Skemer +3
The evolved carbon-rich AGB star IRC +10216 (CW Leo) is the brightest mid-infrared source outside the solar system, as well as one of the closest examples of an evolved star losing…
The First Hundred Brown Dwarfs Discovered by the Wide-field Infrared Survey Explorer (WISE)
J. Davy Kirkpatrick, Michael C. Cushing, Christopher R. Gelino +37
We present ground-based spectroscopic verification of six Y dwarfs (see Cushing et al), eighty-nine T dwarfs, eight L dwarfs, and one M dwarf identified by the Wide-field Infrared…
Dust Grain Evolution in Spatially Resolved T Tauri Binaries
Andrew J. I. Skemer, Laird M. Close, Thomas P. Greene +3
Core-accretion planet formation begins in protoplanetary disks with the growth of small, ISM dust grains into larger particles. The progress of grain growth, which can be quantifie…
Direct Imaging Constraints on the Putative Exoplanet 14 Her c
Timothy J. Rodigas, Jared R. Males, Philip M. Hinz +2
We present results of deep direct imaging of the radial velocity (RV) planet-host star 14 Her (=GJ 614, HD 145675), obtained in the \lprime ~band with the Clio-2 camera and the MMT…
A Combined Subaru/VLT/MMT 1--5 Micron Study of Planets Orbiting HR 8799: Implications for Atmospheric Properties, Masses, and Formation
Thayne Currie, Adam S. Burrows, Yoichi Itoh +9
We present new 1--1.25 micron (z and J band) Subaru/IRCS and 2 micron (K band) VLT/NaCo data for HR 8799 and a rereduction of the 3--5 micron MMT/Clio data first presented by Hinz…