Furthering our knowledge of the solar neighborhood using WISE

Bibcode
2013AN....334...97C
DOI
10.1002/asna.201211754
Dupuy, T. J.; Mace, G. N.; Leggett, S. K.; Lodieu, N.; Gomes, J. I.; Gizis, J. E.; Wright, E. L.; Gelino, C. R.; Kirkpatrick, J. D.; Cushing, M. C.
Bibliographical reference

Astronomische Nachrichten, Vol.334, Issue 1-2, p.97

Advertised on:
2
2013
Number of authors
10
IAC number of authors
1
Citations
0
Refereed citations
0
Description
The launch of NASA's Wide-field Infrared Survey Explorer (WISE) in late 2009 ushered in an new era in the study of the solar neighborhood. Its mid-infrared capabilities have proven critical to the discovery of the bulk of the coolest (\teff < 1000 K) brown dwarfs, including the new Y dwarfs, and its all-sky coverage lends itself to searches for high proper motions stars using other infrared surveys such as the Two Micron All Sky Survey (2MASS), UKIRT Infrared Deep Sky Survey (UKIDSS), and Visible and Infrared Survey Telescope for Astronomy (VISTA) surveys. This splinter session of the 17th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun was organized to bring together researchers working with WISE data to both identify brown dwarfs and characterize their properties.
Related projects
Discovery of a system of super-Earths orbiting the star HD 176986 with about 5.7 and 9.2 Earth masses.
Very Low Mass Stars, Brown Dwarfs and Planets
Our goal is to study the processes that lead to the formation of low mass stars, brown dwarfs and planets and to characterize the physical properties of these objects in various evolutionary stages. Low mass stars and brown dwarfs are likely the most numerous type of objects in our Galaxy but due to their low intrinsic luminosity they are not so
Rafael
Rebolo López
In progress
Type
Refereed
Stellar & Interstellar Physics (FEEI)
Astrometry
Luminosity function
Surveys

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