Abstract
As part of the VISTA Science Verification programme, a large set of
images in Orion was obtained at five near-infrared wavelength bands,
from 0.9 to 2.2 μm. The resulting multi-band catalogue contains
approximately three million sources, allowing investigation of various
issues concerning star and brown dwarf formation, such as a) the
difference in the shape of the substellar mass function in a cluster vs.
non-clustered environment, b) the influence of massive OB stars on the
process of brown dwarf formation, c) the size and morphology of dust
envelopes around protostars, and d) the comparative role of mass and
environment on the evolution of circumstellar discs. The data from the
VISTA Orion Survey, including catalogues, are available to the
community. In this article we present an overview of selected science
results that have emerged so far from this survey.
| Original language | English |
|---|---|
| Pages (from-to) | 29-32 |
| Journal | The Messenger |
| Volume | 145 |
| Publication status | Published - 1 Sept 2011 |
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