Minor Planet Observations [983 San Fernando]
Not Available
Quijano, L. et al.
Fecha de publicación:
10
2005
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Minor Planet Observations [H79 York University Observatory, Toronto]
Not Available
Vaduvescu, O.Fecha de publicación:
102004 -
Model Color-Magnitude Diagrams for Hubble Space Telescope Observations of Local Group Dwarf Galaxies
In this Letter, we discuss a method to conduct a quantitative study of the star formation history (SFH) of Local Group (LG) galaxies using Hubble Space Telescope (HST) data. This method has proved to be successful in the analysis of the SFH of the same kind of galaxies using ground-based observations. It is based on the comparison of observed CMDs
Aparicio, A. et al.Fecha de publicación:
101996 -
Model Comparison for the Density Structure across Solar Coronal Waveguides
The spatial variation of physical quantities, such as the mass density, across solar atmospheric waveguides governs the timescales and spatial scales for wave damping and energy dissipation. The direct measurement of the spatial distribution of density, however, is difficult, and indirect seismology inversion methods have been suggested as an
Arregui, I. et al.Fecha de publicación:
102015 -
Modeling an accretion disk in NGC 985
An optically thick relativistic Keplerian accretion disk model is used to fit the broad component of the H-alpha, H-beta, and He I 5876 A emission line profiles of the active nucleus of NGC 985. A set of values of the relevant parameters is derived from the independent fits of the three lines. Those values are consistent for the lines examined and
Stanga, R. M. et al.Fecha de publicación:
101991 -
Modeling pulsations in hot stars with winds
The interaction pulsation/mass loss takes different aspects. Pulsations can trigger mass loss as in LBVs and Miras; on the other hand, mass loss can modify the driving conditions within the stars. But the most spectacular aspect is the effect on stellar models which, in turn, opens a royal way to asteroseismology to test physical conditions inside
Noels, Arlette et al.Fecha de publicación:
102008