[PDF] Top 20 Autonomía de la voluntad: elección de la ley aplicable al contrato internacional

... Abstract. This paper discusses benchmark brown dwarfs in various environments, and focuses on those in wide binary systems. We present a summary of the recently discovered T dwarf population from the UKIDSS Large ... See full document

... Alamos Stellar pulsation conference on wide field variability ...the infrared) and the somewhat controversial problem of statistical bias in the use of parallaxes (and other methods of distance ...of ... See full document

... the infrared Wide Field Camera 3 (WFC3) on the Hubble Space Telescope (HST), the number of candidates has risen from a few (Bouwens et ...colors, stellar populations (McLure et ... See full document

... the stellar and substellar Initial Mass Function (IMF; [44, 55, 56]) is of prime importance to understand the formation of stars and brown ...a wide range of properties (age, density, environment, etc ... See full document

... the stellar populations we have modelled the spectra extracted from the aper- tures using the evolutionary synthesis models of Gonz´alez Delgado et ...the stellar absorption contributions in ... See full document

... extracted using the Chelex method and the ITS region was amplified in a semi-nested PCR, and sequenced with universal and newly designed primers as described previously 48 ... See full document

... of wide-field infrared imaging in screening, diagnosing, and monitoring structural peripheral retinal disorders including retinoschisis, retinal detachment or combined retinoschi- sis rhegmatogenous ... See full document

... both infrared emission from disks as well as stellar spins to high ...enabled infrared photometry of PMS to detect the presence of disks to unprecedented ... See full document

... for infrared measurements of air temperatures should have especially high emissivity in order to the high accuracy and because of the reduction of the noninfluence of the ambient radiation ...temperature ... See full document

... recent surveys have sought to quantify planet occurrence rates around solar-type FGK stars ...additional stellar companions on the formation and subsequent evolution of planetary systems are not well ...A ... See full document

... The wide luminosity dispersion seen for stars at a given effective temperature in the Hertzsprung–Russell diagrams of young clusters and star-forming regions is often interpreted as due to significant (∼10 Myr) ... See full document

... reduced using the pamela optimal extraction routines (Horne 1986) within the ®garo (Shortridge et ...by using polynomial ®ts to each pixel in the spatial direction, as shown in ...brated using Cu±Ar ... See full document

... velocity field and LOSVDs (see ...ity field is point-symmetric, this is consistent with the accretion of many low-mass ...have stellar masses of at most few 10 8 M ... See full document

... Figure 5. Simplified visual representation of the convolution steps for a full light curve, folded on the best-fitting period. The shading of the boxes represents the different filters that are applied to the data in ... See full document

... the stellar magnetic field that is inclined with respect to the stellar rotation ...magnetic field creates a major funnel flow in each disk hemisphere that interacts with the inner disk, ... See full document

... magnetic field strength of 3T and 4T, the red blood corpuscles and platelets tend to orient ...magnetic field tends to orient which can be attributed to the magnetic ...magnetic field concerning heme ... See full document

... galaxies using integral field spectroscopy data from the Sloan Digital Sky Survey IV Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) ...and stellar population indices demonstrating the ... See full document

... The Zwicky Transient Facility (ZTF) is a next-generation, optical, synoptic survey that leverages the success of the Palomar Transient Factory (PTF). ZTF has a large science focal plane (SFP) that needs to be aligned ... See full document

... There are many interesting and exciting results about exoplanets these days. For example, Galland et al. (2005) found a exoplanet around the F6V star HD33564 showing a strong infrared excess. Baraffe et al. (2005) ... See full document

... new stellar evolution pathways. In some recent work, the use of stellar models which evolve singly but while rotating at a substantial frac- tion of their break-up speed has been explored (for example, this ... See full document