Soft X-Ray Emission and Absorption in Ton 1388

Details Soft X-Ray Emission and Absorption in Ton 1388 Soft X-Ray Emission and Absorption in Ton 1388

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001cxo..prop..959m&link_type=abstract

Chandra Proposal ID #03701000

Computer Science

Chandra Proposal Id #03701000

Scientific paper

We propose to observe the bright Quasi Stellar Object Ton 1388 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 as opposed to continuum absorption edges produced by the warm absorber. Both components will be studied in detail spectroscopically.

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