ACIS Study of Abundance Distribution in ES

Details ACIS Study of Abundance Distribution in ES ACIS Study of Abundance Distribution in ES

Sep 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999cxo..prop..181f&link_type=abstract

Chandra Proposal ID #01600473

Computer Science

Chandra Proposal Id #01600473

Scientific paper

We propose to measure the heavy element abundance distributions for a bright elliptical galaxy NGC5846 and a ram-pressure stripped elliptical in the Virgo cluster, NGC4374 (M84). The AXAF spatial resolution and sensitivity will allow a direct comparison of stellar abundances measured optically with X-ray measurements for the hot corona. These observations will determine the relative contributions to the enrichment of the ISM from different types of supernovae. These measurements also will test various chemical enrichment scenarios.

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