Simultaneous Chandra, HST and Fuse Observations of Warm Absorbers in AGN

Details Simultaneous Chandra, HST and Fuse Observations of Warm Absorbers in AGN Simultaneous Chandra, HST and Fuse Observations of Warm Absorbers in AGN

Jul 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001hst..prop.9275k&link_type=abstract

HST Proposal ID #9275

Computer Science

Hst Proposal Id #9275

Scientific paper

Photoionized, warm absorbing gas is an important component of the nuclear structure of AGN. About half of all low-z AGN show X-ray warm absorbers and high-ionization UV absorption lines, but the relationship of the X-ray absorber to the UV-absorbing gas is not clear. Only a handful of high-spectral-resolution observations with Chandra, HST, or FUSE currently exist {NGC4151, NGC3516, NGC3783, NGC5548, Mrk 509}. These show a diversity of kinematic structure and sample of low-redshift AGN studied at high spectral resolution in the X-ray and the UV by obtaining simultaneous HST, Chandra, and Fuse spectra of Mrk 279. Our HETGS spectra will also probe the origin of narrow Fe Kalpha emission in Seyfert 1s.

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