Secular Evolution in Nearby Galaxies - 1
Not Available
Kormendy, J.
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11
2011
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Secular Evolution in Nearby Galaxies - 2Not AvailableKormendy, J.
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112011 -
Secular Evolution in Nearby Galaxies - 3Not AvailableKormendy, J.
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112011 -
Secular Evolution in Nearby Galaxies - 4Not AvailableKormendy, J.
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112011 -
Seyfert Galaxies at the IR: the ISO perspectiveThe study of the IR emission from Seyfert galaxies is of key importance for understanding the origin of the extraordinary nuclear activity seen in these objects as well as the differences between the various Seyfert types. Two important problems remain unresolved. For instance, whether the IR radiation from Seyfert galaxies is of mostly thermal orPerez Garcia, A. M. et al.
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111998 -
Shape and spin determination of Barbarian asteroidsContext. The so-called Barbarian asteroids share peculiar, but common polarimetric properties, probably related to both their shape and composition. They are named after (234) Barbara, the first on which such properties were identified. As has been suggested, large scale topographic features could play a role in the polarimetric response, if theDevogèle, M. et al.
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112017