Observing brown dwarfs in the Magellanic Cloud star-forming regions with the E-ELT

Details Observing brown dwarfs in the Magellanic Cloud star-forming regions with the E-ELT Observing brown dwarfs in the Magellanic Cloud star-forming regions with the E-ELT

2011-09-28

arxiv.org/abs/1109.6235v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

Proceeding of the RIA Workshop on Gaia "Stellar Clusters & Associations", Granada, May 23-27, 2011

Scientific paper

We present the results of near-infrared imaging simulations of young star-forming regions in the Magellanic Clouds to be observed with the European Extremely Large Telescope (E-ELT). The simulated J,H,K-band images show that we should be able to obtain nearly complete samples of young brown dwarfs above the deuterium burning limit (M > 13 MJup) in low-mass star-forming regions in the Clouds. Moreover, very young giant planet-mass objects in the Clouds should be detectable with the E-ELT under favourable conditions.

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