The Nature of Peculiar Gas Filaments in Early Type Galaxies

Details The Nature of Peculiar Gas Filaments in Early Type Galaxies The Nature of Peculiar Gas Filaments in Early Type Galaxies

Sep 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999cxo..prop...27t&link_type=abstract

Chandra Proposal ID #01600275

Mathematics

Logic

Chandra Proposal Id #01600275

Scientific paper

We propose to address in detail the nature of unexpected morphological similarites between different phases of the ISM in early type galaxies. We aim at obtaining good statistics for detailed morphological comparison in 2 galaxies, NGC 5846 and NGC 1553, for which ROSAT data have already established a close relation between warm and hot gas emission, and at a reliable assessing of the spectral parameters in several regions corresponding to high and low surface brightness features. This study will enable us to establish which is the causal link between optical nebulosity, X-ray emisison from hot gas, and dust in early-type galaxies.

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