Soft X-Ray Emission and Absorption in NGC 4051

Details Soft X-Ray Emission and Absorption in NGC 4051 Soft X-Ray Emission and Absorption in NGC 4051

Sep 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002cxo..prop.1301m&link_type=abstract

Chandra Proposal ID #04700994

Computer Science

Chandra Proposal Id #04700994

Scientific paper

We propose to observe the bright Narrow Line Seyfert 1 galaxy NGC 4051 with the LETG/HRC-S of Chandra. The spectral resolution of the LETGS and its wavelength coverage up to 100 Angstrom allows us to disentangle the contributions of emission features arising from the accretion disk and/or from continuum absorption edges produced by the warm absorber. Both components will be studied in detail, using the spectrosopic as well as the time variability data.

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