Other
Scientific paper
Oct 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007xmm..prop..117b&link_type=abstract
XMM-Newton Proposal ID #05539401
Other
Galaxies, Galactic Surveys, Ngc891, Xmm-Newton Proposal Id #05539401
Scientific paper
We address two important issues by studying the hot gas around the edge-on spiral NGC891. The first issue is the origin of the hot halo, which can occur by infall onto the galaxy or from a galactic fountain generated by disk SNe. We differentiate between models by measuring the gas metallicity, predicted to be low in one model and high in the other. Second, we will measure the vertical component of the galaxy's gravitational field, thereby lifting a degeneracy in mass models and permitting a unique determination of the dark matter density in the baryon-dominated region. We do this by measuring the temperature and emission measure distribution perpendicular to the disk. Existing data prove feasibility but are not sufficiently deep.
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