Resolving the Warm Absorber in NGC 5548

Details Resolving the Warm Absorber in NGC 5548 Resolving the Warm Absorber in NGC 5548

Jul 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001hst..prop.9279k&link_type=abstract

HST Proposal ID #9279

Computer Science

Hst Proposal Id #9279

Scientific paper

We propose to map the ionization and velocity structure of the X-ray and UV absorbers in NGC 5548 with the LETGS and HETGS of Chandra and STIS/HST. NGC 5548 is an important target for this kind of study because 1} it shows multiple kinematic components in the UV characterized by a range in ionization parameter and effective column, 2} it shows evidence for multiple kinematic and ionization components in previous Chandra X-ray spectra, and 3} it has a low Galactic column, which permits coverage of spectral lines out to 80 Angstrom with the LETGS. These data yield the ionization parameter and column density of density of the absorption-line regions as a function of radial velocity, and constrain the elemental abundances and shape of the observered EUV continuum.

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