XMM-Newton Proposal 03049401

Details XMM-Newton Proposal 03049401 XMM-Newton Proposal 03049401

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004xmm..prop..162m&link_type=abstract

XMM-Newton Proposal ID #03049401

Physics

Galaxies, Galactic Surveys, Ngc 1404, Xmm-Newton Proposal 03049401

Scientific paper

The O abundance is the most important, since it is the most abundant element except H and He, and synthesized only by type II supernovae (SNe). In elliptical galaxies, an accumulation of stellar mass loss emit X-rays and therefore, the O abundance of the X-ray emitting gas reflects the stellar metallicity. Therefore, I propose to observe two elliptical galaxies, NGC 1404 and NGC 4374. and determine the O abundance of the gas with the RGS.

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