Journal: Monthly Notices of the Royal Astronomical Society
Publication
Accretion and outflow in V404 Cyg
We study the optical evolution of the 2015 outburst in V404 Cyg, with emphasis on the peculiar nebular phase and subsequent decay to quiescence. From the decay...
Accretion properties of X-ray AGN: evidence for radiation-regulated obscuration with redshift-dependent host galaxy contribution
We adopt a Bayesian X-ray spectral approach to investigate the accretion properties of unobscured ($20\lt \log (N_{\rm H}/{\rm cm}^{-2}\lt 22$) and obscured (...
Accurate fundamental parameters and detailed abundance patterns from spectroscopy of 93 solar-type Kepler targets
We present a detailed spectroscopic study of 93 solar-type stars that are targets of the NASA/Kepler mission and provide detailed chemical composition of each...
Accurate halo-galaxy mocks from automatic bias estimation and particle mesh gravity solvers
Reliable extraction of cosmological information from clustering measurements of galaxy surveys requires estimation of the error covariance matrices of...
Accurate parameters for HD 209458 and its planet from HST spectrophotometry
We present updated parameters for the star HD 209458 and its transiting giant planet. The stellar angular diameter θ = 0.2254 ± 0.0017 mas is obtained from the...
Adaptive optics parameters connection to wind speed at the Teide Observatory
Current projects for large telescopes demand a proper knowledge of atmospheric turbulence to design efficient adaptive optics systems in order to reach large...
Adaptive optics parameters connection to wind speed at the Teide Observatory: corrigendum
García-Lorenzo et al. presented a complete study of atmospheric parameters relevant for adaptive optics in relation to wind speed at the Teide Observatory...
Using N-body simulations, we study the properties of a bar induced in a discy dwarf galaxy as a result of tidal interaction with the Milky Way. The bar forms at...
AGB dust and gas ejecta in extremely metal-poor environments
We present asymptotic giant branch (AGB) models of metallicity Z = 10-4 and 3 × 10-4, with the aim of understanding how the gas enrichment and the dust...