ELMER is an optical instrument for the GTC designed to observe between 3650 and 10000 Armstrong. The observing modes for the instrument at Day One shall be: Imaging, Long Slit Spectroscopy, Mask-multi-object spectroscopy, Slit-less multi-object spectroscopy, Fast Photometry and Fast short-slit spectroscopy. It will be installed at the Nasmyth-B
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Manufacturing, integration, and testing of ELMER structure and mechanismsRonquillo, Bernardo et al.92004
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Mapping the properties of blue compact dwarf galaxies: integral field spectroscopy with PMAS
Context. Blue compact dwarf (BCD) galaxies are low-luminosity, low-metal content dwarf systems undergoing violent bursts of star formation. They present a unique opportunity to probe galaxy formation and evolution and to investigate the process of star formation in a relatively simple scenario. Spectrophotometric studies of BCDs are essential to
Cairós, L. M. et al.Fecha de publicación:
92010 -
Mass Accretion Rate vs. X-ray Luminosity in Low-Mass X-ray Binaries
Not Available
Garcia, M. R.Fecha de publicación:
91987 -
Mass Measurements of Stellar and Intermediate-Mass Black Holes
We discuss the method, and potential systematic effects therein, used for measuring the mass of stellar-mass black holes in X-ray binaries. We restrict our discussion to the method that relies on the validity of Kepler's laws; we refer to this method as the dynamical method. We briefly discuss the implications of the mass distribution of stellar
Casares, J. et al.Fecha de publicación:
92014 -
Massive Clumps in Local Galaxies: Comparisons with High-redshift Clumps
Local UV-bright galaxies in the Kiso survey include clumpy systems with kiloparsec-size star complexes that resemble clumpy young galaxies in surveys at high redshift. We compare clump masses and underlying disks in several dozen galaxies from each of these surveys to the star complexes and disks of normal spirals. Photometry and spectroscopy for
Elmegreen, B. G. et al.Fecha de publicación:
92013 -
Massive relic galaxies prefer dense environments
We study the preferred environments of z ˜ 0 massive relic galaxies (M⋆ ≳ 1010 M⊙ galaxies with little or no growth from star formation or mergers since z ˜ 2). Significantly, we carry out our analysis on both a large cosmological simulation and an observed galaxy catalogue. Working on the Millennium I-WMAP7 simulation we show that the fraction of
Peralta de Arriba, L. et al.Fecha de publicación:
92016