Physical Properties of Low-Luminosity Galaxies at z ~ 2

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dc.creatorLemoine-Busserolle, M.
dc.creatorContini, T.
dc.creatorPello, R.
dc.creatorBorgne, J. -F. Le
dc.creatorKneib, J. -P.
dc.creatorLidman, C.
dc.date2002-07-05
dc.date.accessioned2026-07-07T02:04:11Z
dc.date.available2026-07-07T02:04:11Z
dc.descriptionWe report the results obtained from ISAAC/VLT near-IR spectroscopy of two low-luminosity z ~ 1.9 galaxies located in the core of the lensing cluster AC114. The amplification factor allowed to obtain, for the first time, physical properties (SFR, abundance ratios, mass, etc) of star-forming galaxies, 1 to 2 magnitudes fainter than in previous studies of Lyman-break galaxies at z ~ 3.
dc.description2 pages . To appear in "A Massive Star Odyseey, from Main Sequence to Supernova", Proceedings IAU Symposium No. 212, K.A. van der Hucht, A. Herrero, & C. Esteban (eds)
dc.identifierhttps://arxiv.org/abs/astro-ph/0207141
dc.identifierhttp://arxiv.org/abs/astro-ph/0207141
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4655
dc.subjectAstrophysics
dc.titlePhysical Properties of Low-Luminosity Galaxies at z ~ 2
dc.typetext

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