Optial Surveys for Space Debris in Geo - What about NEOS?
Not Available
Schildknecht, T. et al.
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2001
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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On the Relation between Radio and Non-Radio Elliptical GalaxiesEmpirical evidence suggests that elliptical galaxies hosting a radio source may not be different from normal non-radio ellipticals. To test this possibility, we use Monte Carlo simulations to reproduce the distribution of radio galaxies in the radio-optical luminosity plane. The input parameters of the simulation are the optical luminosity functionScarpa, R. et al.
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On The Parent Population of Radio Galaxies and the FR I--II DichotomyThe possibility of radio galaxies being random sample of otherwise normal elliptical galaxies is tested. Starting with the observed optical luminosity functions for elliptical galaxies, it is shown that the probability of an elliptical forming a radio source is a continuous, increasing function of optical luminosity, precisely proportional toScarpa, R. et al.
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02001 -
On the Origin of the IR Emission in Active Galactic NucleiThe relation between the X-ray, coronal line and IR emission in a sample of the brightest known Seyfert galaxies is analyzed. A close relationship between the absorption-corrected soft X-ray emission and both the mid-IR and the coronal line emission is found for the Seyfert 2-type objects in the sample. The coronal line and X-ray emission bothAlmudena Prieto, M. et al.
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Numerical Simulations of the Ambipolar Filamentation ProcessNot AvailableFranqueira, M. et al.
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Nuclear Star Formation in the Hotspot Galaxy NGC 2903We analyze the star formation properties of the hotspot galaxy NGC 2903 using high resolution Hubble Space Telescope and adaptive optics observations. The circumnuclear star formation in NGC 2903 shows a ringlike morphology with an approximate diameter of 625 pc. For the first time, the infrared hotspots have been resolved into individual youngAlonso-Herrero, A. et al.
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02001