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

  • S. Konami (a1) (a2), K. Matsushita, K. Sato, R. Nagino, N. Isobe, M. S. Tashiro, H. Seta, K. Matsuta, T. Tamagawa and K. Makishima...

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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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References

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Goudfrooij, P., Mack, J., Kissler-Patig, M., Meylan, G., & Minniti, D. 2001a, MNRAS 322, 643
Hayashi, K., Fukazawa, Y., Tozuka, M., Nishino, S., Matsushita, K., Takei, Y., & Arnaud, K. A. 2009, arXiv:0907.2283
Lodders, K. 2003, ApJ 591, 1220
Matsushita, K. et al. 2007, PASJ 59, 327
Tawara, Y., Matsumoto, C., Tozuka, M., Fukazawa, Y., Matsushita, K., & Anabuki, N. 2008, PASJ 60, 307
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Suzaku observation of the metallicity in the interstellar medium of NGC 1316

  • S. Konami (a1) (a2), K. Matsushita, K. Sato, R. Nagino, N. Isobe, M. S. Tashiro, H. Seta, K. Matsuta, T. Tamagawa and K. Makishima...

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