Variability of Quasars at 10 microns

Details Variability of Quasars at 10 microns Variability of Quasars at 10 microns

1999-03-23

arxiv.org/abs/astro-ph/9903363v1

Astronomy and Astrophysics

Astrophysics

AAS LaTex, 33 figures in 2 postscript files, AJ, accepted

Scientific paper

10.1086/300945

Twenty five low redshift quasars have been monitored for several decades at five near- and mid-infrared wavelengths to detect rapid variations which would indicate that a nonthermal component was present in the "10 micron bump". Such variability has apparently been detected in several radio loud quasars and in the radio quiet quasar PG1535+547. In addition, the structure function of PG1226+023 shows that an apparently periodic component is present in its near-infrared emission.

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