Variations in the thermal emission of Seyfert galaxies

Details Variations in the thermal emission of Seyfert galaxies Variations in the thermal emission of Seyfert galaxies

Apr 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980natur.284..410l&link_type=abstract

Nature, Volume 284, Issue 5755, pp. 410-412 (1980).

Physics

72

Scientific paper

Accurate monitoring of five Seyfert galaxies demonstrates that they are
all variable in the IR region. These fluctuations probably arise when
variations in the nonthermal UV sources change the rate of heating of
interstellar dust within the nuclei of these galaxies, as demonstrated
quantitatively for III Zw 2.

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