Suzaku observation of the metallicity in the interstellar medium of NGC 1316

Details Suzaku observation of the metallicity in the interstellar medium of NGC 1316 Suzaku observation of the metallicity in the interstellar medium of NGC 1316

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010hia....15..286k&link_type=abstract

Highlights of Astronomy, Volume 15, p. 286-286

Astronomy and Astrophysics

Astronomy

Scientific paper

Metal abundances of the hot X-ray emitting interstellar medium (ISM) include important information to understand the history of star formation and evolution of galaxies. The metals are mainly synthesized by Type Ia (SNe Ia) and stellar mass loss in elliptical galaxies. The productions of stellar mass loss reflect stellar metallicity. SNe Ia mainly product Fe. Therefore, the abundance pattern of ISM can play key role to investigate the metal enrichment history.

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