Nuclear Magnitudes of Short-Period Comets
Not Available
Fernandez, J. A. et al.
Advertised on:
11
1996
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Nuclear magnitudes of short-period comets.Not AvailableFernández, J. A. et al.
Advertised on:
111996 -
Nudos Cometarios EN la nebulosa de la HeliceThe Cometary Knots in the Helix Nebula have shown themselves to be formed of a head which is a photoionized surface, optically thick to Lyman continuum radiation, on the central star facing sides of neutral clumps and a cometary tails photionized by the diffuse radiation field. In this study we will present the results of a photoionization model ofLopez-Martin, L. et al.
Advertised on:
111998 -
Numerical simulation of propagation of the MHD waves in sunspotsWe present results of numerical 3D simulation of propagation of MHD waves in sunspots. We used two self consistent magnetohydrostatic background models of sunspots. There are two main differences between these models: (i) the topology of the magnetic field and (ii) dependence of the horizontal profile of the sound speed on depth. The model withParchevsky, K. et al.
Advertised on:
112010 -
Obscuration in LINERs. The narrow line regionWe studied the nuclear obscuration of galaxies hosting Low Ionization Narrow Emission Regions (LINERs) based on their X-ray and optical emission. X-ray data show that high obscuration is a common property of LINERs, 50% of them are identified as good candidates to be Compton-thick. From the Hα HST-imaging analysis it is found that the largeMasegosa, J. et al.
Advertised on:
112011 -
OBSERVATIOAvailable from the Minor Planet Center.Sanchez, A. et al.
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112003