Zobrazeno 1 - 10
of 23
pro vyhledávání: '"J. C. Muñoz-Cuartas"'
Autor:
J P Carvajal, J C Muñoz-Cuartas
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 521:6075-6088
The Active Asteroids (AAs), are a small population of minor planets with characteristics similar to both asteroids and comets. In the search for the AAs, the analysis of light curves promises to be an efficient approach to identify candidates. In an
Publikováno v:
Revista Mexicana de Astronomía y Astrofísica. 55:273-288
In this work, we explore the idea that substructures like stellar clusters could be formed from the tidal stream produced in galactic minor mergers. We use N -body and SPH simulations of satellite galaxies interacting with a larger galaxy. We study t
Publikováno v:
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2020, 491 (2), pp.1887-1900. ⟨10.1093/mnras/stz2943⟩
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, 491 (2), pp.1887-1900. ⟨10.1093/mnras/stz2943⟩
Mon.Not.Roy.Astron.Soc., 2020, 491 (2), pp.1887-1900. ⟨10.1093/mnras/stz2943⟩
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, 491 (2), pp.1887-1900. ⟨10.1093/mnras/stz2943⟩
We study the formation of polar ring galaxies via minor mergers. We used N-body+hydrodynamics simulations to reproduce the dynamics of the observed system AM 2229-735 that is a minor merger whose interaction signals are those of a progenitor for a po
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a4c2f4073da62d24055823094c37f71a
https://hal.archives-ouvertes.fr/hal-02447938
https://hal.archives-ouvertes.fr/hal-02447938
Publikováno v:
Wave Motion. 98:102624
Finite difference is a well-suited technique for modeling acoustic wave propagation in heterogeneous media as well as for imaging and inversion. Typically, the method aims at solving a set of partial differential equations for the unknown pressure fi
Autor:
J. C. Muñoz-Cuartas, Sheryl Avendaño
Publikováno v:
CT&F-Ciencia, Tecnología y Futuro, Volume: 8, Issue: 2, Pages: 47-56, Published: DEC 2018
Seismic modeling is an important step in the process used for imaging Earth subsurface. Current applications require accurate models associated with solutions of the wave propagation equation in real media. Unfortunately, it is common not to find in
Publikováno v:
Chaos, Solitons & Fractals. 82:22-33
The dark matter halo distribution of the nearby universe is used to study the fractal behaviour in the proximate universe. The data, which is based on four volume-limited galaxy samples was obtained by Munoz-Cuartas and Mueller (2012) from the Sevent
Autor:
Tiit Sepp, Meghan E. Gray, Lyndsay Old, Volker Müller, Steven P. Bamford, R. R. de Carvalho, Darren J. Croton, J. C. Muñoz-Cuartas, Daniel Gifford, Eli S. Rykoff, Gary A. Mamon, R. J. Pearson, Cristóbal Sifón, A. von der Linden, A. Saro, R. A. Skibba, Elmo Tempel, Frazer R. Pearce, R. Wojtak, Eduardo Rozo
Publikováno v:
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2018, 481 (1), pp.324-340. ⟨10.1093/mnras/sty2257⟩
Monthly Notices of the Royal Astronomical Society
Mon.Not.Roy.Astron.Soc., 2018, 481 (1), pp.324-340. ⟨10.1093/mnras/sty2257⟩
Monthly Notices of the Royal Astronomical Society
The primary difficulty in measuring dynamical masses of galaxy clusters from galaxy data lies in the separation between true cluster members from interloping galaxies along the line of sight. We study the impact of membership contamination and incomp
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::95ead87d87b521a7b2933062df37de77
https://hal.archives-ouvertes.fr/hal-01823296
https://hal.archives-ouvertes.fr/hal-01823296
Publikováno v:
Brazilian Journal of Geophysics. 37:131
Seismic modeling is an important step in the process used for imaging Earth sub-surface. Current applications require accurate models associated with solutions of the equation of wave propagation in realistic medium. In this work, we propose a modeli
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 428:882-890
We analyze the properties of dark matter halos in the cold-plus-warm dark matter cosmologies (CWDM). We study their dependence on the fraction and velocity dispersion of the warm particle, keeping the free-streaming scale fixed. To this end we consid
Autor:
Volker Müller, J. C. Muñoz-Cuartas
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 423:1583-1595
In this work we introduce a new method to perform the identification of groups of galaxies and present results of the identification of galaxy groups in the seventh data release of the Sloan Digital Sky Survey. Our methodology follows an approach tha