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Además ofrece acceso al repositorio de preprints del IAC: https://research.iac.es/preprints/l
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The EDGE-CALIFA Survey: Interferometric Observations of 126 Galaxies with CARMAWe present interferometric CO observations, made with the Combined Array for Millimeter-wave Astronomy (CARMA) interferometer, of galaxies from the Extragalactic Database for Galaxy Evolution survey (EDGE). These galaxies are selected from the Calar Alto Legacy Integral Field Area (CALIFA) sample, mapped with optical integral field spectroscopyBolatto, A. D. et al.
Fecha de publicación:
92017 -
The effect of baryons on the inner density profiles of rich clustersWe use the `Evolution and assembly of galaxies and their environments' (EAGLE) cosmological simulation to investigate the effect of baryons on the density profiles of rich galaxy clusters. We focus on EAGLE clusters with M200 > 1014 M⊙ of which we have six examples. The central brightest cluster galaxies (BCGs) in the simulation have steep stellarMcCarthy, I. G. et al.
Fecha de publicación:
92015 -
The Effect of the Relative Orientation between the Coronal Field and New Emerging Flux. I. Global PropertiesThe emergence of magnetic flux from the convection zone into the corona is an important process for the dynamical evolution of the coronal magnetic field. In this paper we extend our previous numerical investigations, by looking at the process of flux interaction as an initially twisted flux tube emerges into a plane-parallel, coronal magneticGalsgaard, K. et al.
Fecha de publicación:
92007 -
The Effects of Magnetic-field Geometry on Longitudinal Oscillations of Solar ProminencesWe investigate the influence of the geometry of the solar filament magnetic structure on the large-amplitude longitudinal oscillations. A representative filament flux tube is modeled as composed of a cool thread centered in a dipped part with hot coronal regions on either side. We have found the normal modes of the system and establish that theLuna, M. et al.
Fecha de publicación:
92012 -
The effects of magnetic-field geometry on longitudinal oscillations of solar prominences: Cross-sectional area variation for thin tubesContext. Solar prominences are subject to both field-aligned (longitudinal) and transverse oscillatory motions, as evidenced by an increasing number of observations. Large-amplitude longitudinal motions provide valuable information on the geometry of the filament-channel magnetic structure that supports the cool prominence plasma against gravityLuna, M. et al.
Fecha de publicación:
92016