The Distribution of Elements between Gas and Dust in the Interstellar Line of Sight toward X Persei

Details The Distribution of Elements between Gas and Dust in the Interstellar Line of Sight toward X Persei The Distribution of Elements between Gas and Dust in the Interstellar Line of Sight toward X Persei

May 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aas...200.7308d&link_type=abstract

American Astronomical Society, 200th AAS Meeting, #73.08; Bulletin of the American Astronomical Society, Vol. 34, p.767

Astronomy and Astrophysics

Astronomy

Scientific paper

We present results of elemental abundance measurements in the interstellar medium along a line of sight to X Persei (aka HD 24534/4U 0352 +30). Using high S/N spectrscopic UV data obtained using HST-STIS, we measured line profiles and equivalent widths to determine column densities and depletions in the gas. We compare these results with those obtained from Chandra x-ray data for total abundances and depletions of the medium along the same line of sight and discuss the overall distribution of the elements between the gas and the dust.

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