Zobrazeno 1 - 10
of 313
pro vyhledávání: '"Gavilán, M."'
Autor:
Castilla-Gavilán, M., Muñoz-Martínez, M., Zuasti, E., Canoura-Baldonado, J., Mondoñedo, R., Hachero-Cruzado, I.
Publikováno v:
In Aquaculture 30 March 2024 583
First report of frequencies of Y chromosome microdeletions at a reproductive medicine center in Peru
Publikováno v:
In Heliyon October 2023 9(10)
Publikováno v:
In Aquaculture 30 August 2023 573
Autor:
Bellocchi, E., Ascasibar, Y., Galbany, L., Sanchez, S. F., Ibarra-Medel, H., Gavilan, M., Diaz, A.
Publikováno v:
A&A 625, A83 (2019)
We study how the use of several stellar subtraction methods and line fitting approaches can affect the derivation of the main kinematic parameters (velocity and velocity dispersion fields) of the ionized gas component. The target of this work is the
Externí odkaz:
http://arxiv.org/abs/1903.06252
Akademický článek
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This work studies the relation between gas-phase oxygen abundance and stellar-to-gas fraction in nearby galaxies. We first derive the theoretical prediction, and argue that this relation is fundamental, in the sense that it must be verified regardles
Externí odkaz:
http://arxiv.org/abs/1406.6397
Autor:
Molla, M., Gavilan, M.
We carefully analyze how the abundance of Nitrogen over Oxygen evolves when dependent on metallicity stellar yields with a primary component of N proceeding from AGBs stars are used. We show the results obtained with a chemical evolution models grid,
Externí odkaz:
http://arxiv.org/abs/1004.0754
We have developed a grid of chemical evolution models applied to dwarf isolated galaxies, using \cite{gav05} yields. The input data enclose different star formation efficiencies, galaxy mass and collapse time values. The result is a wide collection o
Externí odkaz:
http://arxiv.org/abs/0903.0932
We analyze the evolution of nitrogen resulting from a set of spiral and irregular galaxy models computed for a large number of input mass radial distributions and with various star formation efficiencies. We show that our models produce a nitrogen ab
Externí odkaz:
http://arxiv.org/abs/0711.3133
Publikováno v:
Mon.Not.Roy.Astron.Soc.372:1069-1080,2006
The main objective of the present work is to ckeck if the star formation efficiency plays a relevant role in the evolution of the relative abundance N/O. We analyze the evolution of the nitrogen-to-oxygen ratio as predicted by a set of computed theor
Externí odkaz:
http://arxiv.org/abs/astro-ph/0608214