Dusty warm absorbers: The case of IRAS 13349+2438

Details Dusty warm absorbers: The case of IRAS 13349+2438 Dusty warm absorbers: The case of IRAS 13349+2438

1999-06-24

arxiv.org/abs/astro-ph/9906377v1

Astrophys.Space Sci. 272 (2000) 299-302

Astronomy and Astrophysics

Astrophysics

4 pages incl. 2 figures (needs crckapb.sty); contribution to the proc. of `Astrophysical Dynamics' (Evora, April 14-16, 1999),

Scientific paper

10.1023/A:1002669118194

Warm absorbers are an important new probe of the central region of active galaxies (AGN). Observing and modeling this component provides a wealth of information on the nature of the warm absorber itself, its relation to other components of the active nucleus, and the intrinsic AGN X-ray spectral shape. We briefly review the general properties of dusty warm gas. For the first time, we then apply such a model to the IR loud quasar IRAS 13349+2438. It was the first to be suggested to host a dusty warm absorber (Brandt et al. 1996), but has not yet been modeled as such.

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