NPARSEC: NTT Parallaxes of Southern Extremely Cool objects. Goals, targets, procedures and first results
Author
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Smart, R. L.
Author
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Tinney, C. G.
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Author
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Bucciarelli, B.
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Marocco, F.
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Abbas, U.
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Andrei, A.
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Author
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Bernardi, G.
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Burningham, B.
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Author
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Cardoso, C.
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Costa Hechenleitner, Edgardo
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Author
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Crosta, M. T.
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Daprá, A.
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Day Jones, A.
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Goldman, B.
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Jones, H. R.
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Lattanzi, M. G.
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Author
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Leggett, S. K.
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Author
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Lucas, P.
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Author
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Méndez Bussard, René Alejandro
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Author
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Penna, J. L.
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Author
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Pinfield, D.
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Author
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Smith, L.
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Author
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Sozzetti, A.
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Author
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Vecchiato, A.
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Admission date
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2014-03-06T19:36:53Z
Available date
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2014-03-06T19:36:53Z
Publication date
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2013
Cita de ítem
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MNRAS 433, 2054–2063 (2013)
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Identifier
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doi:10.1093/mnras/stt876
Identifier
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https://repositorio.uchile.cl/handle/2250/126413
General note
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Artículo de publicación ISI
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Abstract
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The discovery and subsequent detailed study of T dwarfs have provided many surprises and
pushed the physics and modelling of cool atmospheres in unpredicted directions. Distance
is a critical parameter for studies of these objects to determine intrinsic luminosities, test
binarity and measure their motion in the Galaxy.We describe a new observational programme
to determine distances across the full range of T-dwarf subtypes using the New Technology
Telescope (NTT)/SOFI telescope/instrument combination. We present preliminary results for
ten objects, five of which represent new distances.
en_US
Lenguage
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en
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Publisher
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Oxford University Press on behalf of the Royal Astronomical Society