HIGH-RESOLUTION SPECTROSCOPY OF A YOUNG, LOW-METALLICITY OPTICALLY THIN L = 0.02L STAR-FORMING GALAXY AT z = 3.12

HIGH-RESOLUTION SPECTROSCOPY OF A YOUNG, LOW-METALLICITY OPTICALLY THIN L = 0.02L STAR-FORMING GALAXY AT z = 3.12

We present VLT/X-Shooter and MUSE spectroscopy of a faint F814W = 28.60 + or - 0.33 (M sub(UV)=-17.0, low-mass ([

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Bibliographische Detailangaben
Veröffentlicht in:Astrophysical journal. Letters 2016-04, Vol.821 (2), p.L27-L27
Hauptverfasser: Vanzella, E, De Barros, S, Cupani, G, Karman, W, Gronke, M, Balestra, I, Coe, D, Mignoli, M, Brusa, M, Calura, F
Format: Artikel
Sprache:eng
Schlagworte:
ABUNDANCE
ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
COSMIC DUST
Emission
Fluxes
Galaxies
GALAXY CLUSTERS
GRAVITATIONAL LENSES
High resolution
HYDROGEN
Interstellar matter
Ionization
IONIZING RADIATIONS
LUMINOSITY
METALLICITY
OXYGEN
RED SHIFT
SIGNAL-TO-NOISE RATIO
SPECTROSCOPY
Star formation
STARS
TELESCOPES
ULTRAVIOLET RADIATION
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Beschreibung
Zusammenfassung:We present VLT/X-Shooter and MUSE spectroscopy of a faint F814W = 28.60 + or - 0.33 (M sub(UV)=-17.0, low-mass ([
ISSN:2041-8205
2041-8213
DOI:10.3847/2041-8205/821/2/L27