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Cepheid distances from the SpectroPhoto-Interferometry of Pulsating Stars (SPIPS) Application to the prototypes delta Cephei and eta Aquilae
(EDP Sciences, 2015)
Context. The parallax of pulsation, and its implementations such as the Baade-Wesselink method and the infrared surface brightness technique, is an elegant method to determine distances of pulsating stars in a quasi-geometrical ...
A Resolved and Asymmetric Ring of PAHs within the Young Circumstellar Disk of IRS 48
(IOP Publishing, 2017)
For one decade, the spectral type and age of the rho Oph object IRS-48 were subject to debate. and mystery. Modeling its disk with mid-infrared to millimeter observations led to various explanations to account for the ...
. Plataforma tecnológica para optimizar la planeación urbana en la ciudad de Guayaquil dirigido a la transportación, enfocado a la propuesta de implementación y administración de infraestructura Cloud para el proyecto Lesstraffic.
(Universidad de Guayaquil Facultad de Ciencias Matemáticas y Físicas Carrera de Ingeniería en Sistemas Computacionales, 2019-04)
El proyecto LESSTRAFFIC levantó su infraestructura en la nube alojándola en Amazon Web Services, en la primera fase no se llevó un adecuado control de la
administración, lo cual desencadenó en altos consumos y despilfarro ...
A measure of the size of the magnetospheric accretion region in TW Hydrae
(Nature Publishing Group (Nature Research), 2020)
Stars form by accreting material from their surrounding disks. There is a consensus that matter flowing through the disk is channelled onto the stellar surface by the stellar magnetic field. This is thought to be strong ...
The GRAVITY young stellar object survey VI. Mapping the variable inner disk of HD 163296 at sub-au scales
(EDP Sciences, 2021)
Context. Protoplanetary disks drive some of the formation process (e.g., accretion, gas dissipation, formation of structures) of stars and planets. Understanding such physical processes is one of the most significant ...