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Two-dimensional hydrodynamic models of super star clusters with a positive star formation feedback
(The astrophysical journal, 2008)
Optical photometry and spectroscopy of the 1987A-like supernova 2009mw
(Wiley Blackwell Publishing, Inc, 2016-06)
We present optical photometric and spectroscopic observations of the 1987A-like supernova (SN) 2009mw. Our BV RI and g ′ r ′ i ′ z ′ photometry covers 167 days of evolution, including the rise to the light curve maximum, ...
Protoplanetary Disks Including Radiative Feedback from Accreting Planets
(The American Astronomical Society, 2015)
While recent observational progress is converging on the detection of compact regions of thermal emission due to
embedded protoplanets, further theoretical predictions are needed to understand the response of a ...
Black hole fuelling in galaxy mergers: a high-resolution analysis
(Oxford, 2021)
Using parsec scale resolution hydrodynamical adaptive mesh refinement simulations, we have studied the mass transport process throughout a Galactic merger. The aim of such study is to connect both the peaks of mass accretion ...
The stellar metallicity gradients in galaxy discs in a cosmological scenario
(2016)
Context. The stellar metallicity gradients of disc galaxies provide information on disc assembly, star formation processes, and chemical evolution. They also might store information on dynamical processes that could affect ...
DNA Interaction with diaminobenzidine studied with optical tweezers and dynamic light scattering
(The Journal of Physical Chemistry B, 2018)
Mass discrepancy analysis for a select sample of Type II-Plateau supernovae
(EDP Sciences, 2019-09-16)
The detailed study of supernovae (SNe) and their progenitors allows a better understanding of the evolution of massive stars and how these end their lives. Despite its importance, the range of physical parameters for the ...
Delaunay triangulations for moving points fixed radius near neighbors
(Universidad de Chile, 2021)
En simulaciones de fluidos basadas en el método smoothed particle hydrodynamics (SPH), la operación para encontrar los vecinos dado un cierto umbral fijo de cada partícula es la operación más costosa que debe realizarse ...
Horseshoe drag in three-dimensional globally isothermal disks
(IOP Publishing, 2016-01)
We study the horseshoe dynamics of a low-mass planet in a three-dimensional, globally isothermal, inviscid disk. We find, as reported in previous work, that the boundaries of the horseshoe region (separatrix sheets) have ...