Erratum: Structure and star formation in disc galaxies - I. Sample selection and near-infrared imaging
Not Available
Knapen, J. H. et al.
Advertised on:
11
2003
This section contains the publications database that collects IAC articles published in scientific journals. Please, click on the arrow to see full search filter and sort options: author, journal, year, etc..
It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/
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Erratum: A modified χ2-test for cosmic microwave background analysesNot AvailableRubiño-Martín, J. A. et al.
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112003 -
Dynamo action in turbulent flowsWe present results from numerical simulations of nonlinear MHD dynamo action produced by three-dimensional flows that become turbulent for high values of the fluid Reynolds number. The magnitude of the forcing function driving the flow is allowed to evolve with time in such way as to maintain an approximately constant velocity amplitude (andArchontis, V. et al.
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112003 -
Constraints on lepton flavor violation in the two Higgs doublet modelConstraints on the whole spectrum of lepton flavor violating vertices are shown in the context of the standard two Higgs doublet model. The vertex involving the $e- au$ mixing is much more constrained than the others, and the decays proportional to such vertex are usually very suppressed.Diaz, Rodolfo A. et al.
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112003 -
CCC Observations of Pluto, Neptune and Triton with the San Fernando automatic meridian circle.The San Fernando automatic meridian circle (CMASF) is a meridian telescope built by Grubb-Parsons in 1948 fully automated between 1987 and 1995. In 1996 was moved from the Real Instituto y Observatorio de la Armada (ROA) in San Fernando to the Carlos U. Cesco (CUC) mountain observatory in San Juan (Argentine). The CUC is owned by the ObservatorioMuiños, J. L. et al.
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Análisis sismológico de las estrellas pulsantes tipo Delta Scuti del cúmulo de las PléyadesThe seismological analysis of Delta Scuti stars give us precise information on the stellar structure in intermediate mass stars, that is between 1.5 and 2.5 Msun. These variable stars are suitable candidates for probing some of the hydrodynamical processes, actually poorly understood, occurring in the deep interior of the stars. On the other handFox Machado, L.
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112003