Zobrazeno 1 - 10
of 31
pro vyhledávání: '"Bignone, Lucas"'
Autor:
Cataldi, Pedro, Pedrosa, Susana, Tissera, Patricia, Artale, Maria Celeste, Padilla, Nelson, Dominguez-Tenreiro, Rosa, Bignone, Lucas, Gonzalez, Roberto, Pellizza, Leonardo
In this work, we aim at investigating the morphology evolution of Milky Way mass-like dark matter haloes selected from the CIELO and IllustrisTNG Projects. The connection between halo shapes and their environment has been studied in previous works at
Externí odkaz:
http://arxiv.org/abs/2302.08853
Autor:
Santos-Santos, Isabel, Gámez-Marín, Matías, Domínguez-Tenreiro, Rosa, Tissera, Patricia B., Bignone, Lucas, Pedrosa, Susana E., Artal, Héctor, Gómez-Flechoso, M. Ángeles, Rufo-Pastor, Víctor, Martínez-Serrano, Francisco, Serna, Arturo
We use two zoom-in $\Lambda$CDM hydrodynamical simulations of massive disk galaxies to study the possible existence of fixed satellite groups showing a kinematically-coherent behaviour across evolution (angular momentum conservation and clustering).
Externí odkaz:
http://arxiv.org/abs/2211.04491
Autor:
Tissera, Patricia B., Rosas-Guevara, Yetli, Sillero, Emanuel, Pedrosa, Susana E., Theuns, Tom, Bignone, Lucas
We analyse the evolution of the oxygen abundance gradient of star-forming galaxies with stellar mass Mstar > 10^9 Mo in the EAGK simulation over the redshift range z=[0, 2.5]. We find that the median metallicity gradient of the simulated galaxies is
Externí odkaz:
http://arxiv.org/abs/2112.06553
Autor:
Varela-Lavin, Silvio, Tissera, Patricia B., Gómez, Facundo A., Bignone, Lucas A., Lagos, Claudia del P.
Observations show that the surface brightness of disc galaxies can be well-described by a single exponential (TI), up-bending (TIII) or down-bending (TII) profiles in the outskirts. Here we characterize the mass surface densities of simulated late-ty
Externí odkaz:
http://arxiv.org/abs/2111.14126
Autor:
Santos-Santos, Isabel, Dominguez-Tenreiro, Rosa, Artal, Hector, Pedrosa, Susana E., Bignone, Lucas, Martinez-Serrano, Francisco, Gomez-Flechoso, M. Angeles, Tissera, Patricia B., Serna, Arturo
We address the 'plane of satellites problem' by studying planar configurations around two disc galaxies with no late major mergers, formed in zoom-in hydro-simulations. Due to the current lack of good quality kinematic data for M31 satellites, we use
Externí odkaz:
http://arxiv.org/abs/2004.11585
Autor:
Bignone, Lucas A., Pedrosa, Susana E., Trayford, James W., Tissera, Patricia B., Pellizza, Leonardo J.
We study the optical morphology of galaxies in a large-scale hydrodynamic cosmological simulation, the EAGLE simulation. Galaxy morphologies were characterized using non-parametric statistics (Gini, $M_{20}$, Concentration and Asymmetry) derived from
Externí odkaz:
http://arxiv.org/abs/1908.10936
We identify a simulated Milky Way analog in the EAGLE suite of cosmological hydrodynamical simulations. This galaxy not only shares similar global properties as the Milky Way, but was specifically selected because its merger history resembles that cu
Externí odkaz:
http://arxiv.org/abs/1908.07080
Publikováno v:
MNRAS 469 (2017) 4921-4932
We study the properties of long gamma-ray bursts (LGRBs) using a large scale hydrodynamical cosmological simulation, the Illustris simulation. We determine the LGRB host populations under different thresholds for the LGRB progenitor metallicities, ac
Externí odkaz:
http://arxiv.org/abs/1706.03772
Autor:
Bignone, Lucas A., Tissera, Patricia B., Sillero, Emanuel, Pedrosa, Susana E., Pellizza, Leonardo J., Lambas, Diego G.
Publikováno v:
Monthly Notices of the Royal Astronomical Society, Volume 469, Issue 4, 21 August 2017
We study non-parametric morphologies of mergers events in a cosmological context, using the Illustris project. We produce mock g-band images comparable to observational surveys from the publicly available Illustris simulation idealized mock images at
Externí odkaz:
http://arxiv.org/abs/1610.02416
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.