High Resolution Observations of X-ray Absorbers/Emitters

2; (2) Osservatorio Astronomico di Monteporzio; 3); (3) Istituto di Astrofisica Spaziale -- CNR; (4) Universita' degli Studi Roma-3); F. Fiore (2); F. Nicastro (1; G. Matt (4); M. Elvis (1); S. Savaglio (2) ((1) Harvard-Smithsonian Center for Astrophysics

arxiv: astro-ph/0007050 · v1 · submitted 2000-07-05 · 🌌 astro-ph

High Resolution Observations of X-ray Absorbers/Emitters

F. Nicastro (1 , 2 , 3) , M. Elvis (1) , F. Fiore (2) , G. Matt (4) , S. Savaglio (2) ((1) Harvard-Smithsonian Center for Astrophysics , (2) Osservatorio Astronomico di Monteporzio

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(3) Istituto di Astrofisica Spaziale -- CNR (4) Universita' degli Studi Roma-3)

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keywords absorbersemitterstypewarmx-rayabsorptionapplicationbackground

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We present photoionization and collisional ionization models, and their application to three important fields: (a) the Warm Absorbers/Emitters in type 1 AGN, (b) the Warm Reflectors in Type 2 AGN, and (c) X-ray absorption of background quasars by intergalactic gas. A number of cases are investigated, and the dependences of the main parameters explored.

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High Resolution Observations of X-ray Absorbers/Emitters

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