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pro vyhledávání: '"Mejía, J."'
Autor:
León, Federico, Bustamante, María, Mejía, J. Enrique, Ramos, Miguel, Mostajo, Eduardo, Monge, Rosa
Publikováno v:
Revista de Psicología. 9(1):103-115
In order to counsel clients, provide methods, and make clinical references INPPARES' community promoters of contraceptives must know family planning technology. This article describes the construction of the Family Planning Knowledge Test for Promoto
Externí odkaz:
http://revistas.pucp.edu.pe/index.php/psicologia/article/view/3800/3777
http://repositorio.pucp.edu.pe/index/handle/123456789/101641
http://repositorio.pucp.edu.pe/index/handle/123456789/101641
Autor:
Lambert, T. S., Posses, A., Aravena, M., Gónzalez-López, J., Assef, R. J., Díaz-Santos, T., Brisbin, D., Decarli, R., Herrera-Camus, R., Mejía, J., Ricci, C.
High-redshift observations are often biased towards massive and bright galaxies that are not necessarily representative of the full population. In order to accurately study galaxy evolution and mass assembly at these redshifts, observations of ``norm
Externí odkaz:
http://arxiv.org/abs/2210.10023
Autor:
Burkhart, B., Appel, S., Bialy, S., Cho, J., Christensen, A. J., Collins, D., Federrath, C., Fielding, D., Finkbeiner, D., Hill, A. S., Ibanez-Mejia, J. C., Krumholz, M. R., Lazarian, A., Li, M., Mocz, P., Mac Low, M. -M., Naiman, J., Portillo, S. K. N., Shane, B., Slepian, Z., Yuan, Y.
Turbulence is a key process in many fields of astrophysics. Advances in numerical simulations of fluids over the last several decades have revolutionized our understanding of turbulence and related processes such as star formation and cosmic ray prop
Externí odkaz:
http://arxiv.org/abs/2010.11227
Theories suggest that filament fragmentation should occur on a characteristic fragmentation length-scale. This fragmentation length-scale can be related to filament properties, such as the width and the dynamical state of the filament. Here we presen
Externí odkaz:
http://arxiv.org/abs/1901.06205
Akademický článek
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We present synthetic dust polarisation maps of 3D magneto-hydrodynamical simulations of molecular clouds before the onset of stellar feedback. The clouds are modelled within the SILCC-Zoom project and are embedded in their galactic environment. The r
Externí odkaz:
http://arxiv.org/abs/1804.10157
Publikováno v:
A&A 610, A62 (2018)
The fragmentation of filaments in molecular clouds has attracted a lot of attention as there seems to be a relation between the evolution of filaments and star formation. The study of the fragmentation process has been motivated by simple analytical
Externí odkaz:
http://arxiv.org/abs/1711.01417