Chandra Constraints on the Column Density to XTE J1817-330

Details Chandra Constraints on the Column Density to XTE J1817-330 Chandra Constraints on the Column Density to XTE J1817-330

Feb 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006atel..746....1m&link_type=abstract

The Astronomer's Telegram, #746

Astronomy and Astrophysics

Astronomy

6

X-Ray, Binaries, Black Holes, Transients

Scientific paper

We observed the black hole candidate with Chandra for 50 ksec, starting on Feb 13 2006 at 02:04 UT. The HETGS was used to obtain a high resolution spectrum, which was read-out with the ACIS-S array. Initial fits to the spectra have been made using XSPEC and ISIS. For a number of continuum models, and neutral absorption models, we find N_H = 8.8-9.7 E+20 cm^-2. This value is even lower than that anticipated in ATEL 743.

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