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The Origin of the Stellar Mass Distribution and Multiplicity
(Springer, 2020)
Possible link between the power spectrum of interstellar filaments and the origin of the prestellar core mass function
(EDP Sciences, 2015)
A complete understanding of the origin of the prestellar core mass function (CMF) is crucial. Two major features of the prestellar CMF are 1) a broad peak below 1M(circle dot), presumably corresponding to a mean gravitational ...
THE PHYSICAL AND KINEMATICAL STRUCTURE OF MASSIVE AND DENSE COLD CORES
(2019)
In spite of the efforts focused on understanding the formation of high mass stars, we do not have a clear understanding of which are the processes involved. To understand it, we need to characterize objects in very early ...
Resolving the core of R136 in the optical
(IOP Publishing, 2022)
The sharpest optical images of the R136 cluster in the Large Magellanic Cloud are presented, allowing us for the first
time to resolve members of the central core, including R136a1, the most-massive star known. These data ...
Fuerzas nucleares con centro repulsivo y el modelo de capas de núcleo. Efectos de segundo orden
(Revista Mexicana de Física, 2009)