Zobrazeno 1 - 10
of 144
pro vyhledávání: '"ESPINOSA, Martín"'
Autor:
BARROS, Lucas A.1,2, ESPINOSA, Martín3,4, ROMERO, Oscar E.1,2, CARRIZO, Adrian5, CAVALLO, María J.1, DIEZ, Patricia A.1,4 diezpatriciaa@gmail.com
Publikováno v:
Revista de la Sociedad Entomológica Argentina. jul-sep2024, Vol. 83 Issue 3, p29-33. 5p.
Publikováno v:
In BBA - Molecular Basis of Disease January 2024 1870(1)
We perform direct numerical simulations of rotating turbulent Waleffe flow, the flow between two parallel plates with a sinusoidal streamwise shear driving force, to study the formation of large-scale structures and the mechanisms for momentum transp
Externí odkaz:
http://arxiv.org/abs/1903.10652
Publikováno v:
Revista de la Sociedad Entomológica Argentina. ene-mar2024, Vol. 83 Issue 1, p54-57. 4p.
We present a detailed hydrodynamic model that matches the present structure of the well-observed preplanetary nebula OH231.8+04.2. The purpose of the model is to present a physically justified and coherent picture of its evolutionary history from abo
Externí odkaz:
http://arxiv.org/abs/1706.01516
Autor:
Ana Gabriela Díaz Espinoza, Jeanneth Patricia Tapia Cárdenas, Tania Ximena Cajamarca Cárdenas, Zoila Katherine Salazar Torres, Lizette Espinosa Martín
Publikováno v:
QhaliKay, Vol 7, Iss 1 (2023)
Externí odkaz:
https://doaj.org/article/eaefc8c1f4404c97a22ace3334eb6230
Publikováno v:
In Biological Control September 2021 160
Akademický článek
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Autor:
Blackman, Eric G., Carroll-Nellenback, Jonathan J., Frank, Adam, Huarte-Espinosa, Martin, Nordhaus, Jason
Binary systems consisting of a secondary accreting form a wind-emitting primary are ubiquitous in astrophysics. The phenomenology of such Bondi-Hoyle-Lyttleton (BHL) accretors is particularly rich when an accretion disc forms around the secondary. Th
Externí odkaz:
http://arxiv.org/abs/1308.4198
Autor:
Balick, Bruce, Huarte-Espinosa, Martín, Frank, Adam, Gomez, Thomas, Alcolea, Javier, Corradi, Romano L. M., Vinković, Dejan
Our ultimate goal is to probe the nature of the collimator of the outflows in the pre PN CRL618. CRL618 is uniquely suited for this purpose owing to its multiple, bright, and carefully studied finger-shaped outflows east and west of its nucleus. We c
Externí odkaz:
http://arxiv.org/abs/1305.5304