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Título:
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Clumpy Galaxies in CANDELS. II. Physical Properties of UV-bright Clumps at 0.5
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Autores:
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Pérez González, Pablo Guillermo ;
otros, ...
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Tipo de documento:
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texto impreso
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Editorial:
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American Astronomical Society, 2018-02-01
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Dimensiones:
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application/pdf
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Nota general:
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info:eu-repo/semantics/openAccess
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Idiomas:
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Palabras clave:
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Estado = Publicado
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Materia = Ciencias: Física: Astrofísica
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Materia = Ciencias: Física: Astronomía
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Tipo = Artículo
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Resumen:
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Studying giant star-forming clumps in distant galaxies is important to understand galaxy formation and evolution. At present, however, observers and theorists have not reached a consensus on whether the observed "clumps" in distant galaxies are the same phenomenon that is seen in simulations. In this paper, as a step to establish a benchmark of direct comparisons between observations and theories, we publish a sample of clumps constructed to represent the commonly observed "clumps" in the literature. This sample contains 3193 clumps detected from 1270 galaxies at 0.5
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En línea:
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https://eprints.ucm.es/47065/1/perezgonzalez172libre.pdf
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