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Suzaku observations of early-type galaxies

  • K. Matsushita (a1), Y. Fukazawa (a2), K. Hayashi (a2), S. Konami (a1), R. Nagino (a1), T. Ohashi (a3), Y. Tawara (a4) and M. Tozuka (a1)...

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The metal abundances in the hot X-ray emitting interstellar medium (ISM) of early-type galaxies give us important information about the present metal supply into the ISM through supernovae (SNe) Ia and stellar mass loss. In addition, O and Mg abundances should reflect the stellar metallicity and enable us to directly look into the formation history of these galaxies. The XIS instrument onboard the Suzaku satellite has an improved line spread function due to a very small low-pulse-height tail below 1 keV coupled with a very low background.

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References

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Hayashi, K., Fukazawa, Y., Tozuka, M., Nishino, S., Matsushita, K., Takei, Y., & Arnaud, K. A. 2009, PASJ in press, arXiv:0907.2283
Konami, S., in preparation
Lodders, K. et al. 2003, ApJ 591, 1220
Matsushita, K., Finoguenov, A., & Böhringer, H. 2003, A&A 401, 443
Matsushita, K. et al. 2007a, PASJ 59, 327
Matsushita, K., Böhringer, H., Takahashi, I., & Ikebe, Y. 2007b, A&A 462, 953
Nagino, R. & Matsushita, K. in preparation
Tawara, Y., Matsumoto, C., Tozuka, M., Fukazawa, Y., Matsushita, K., & Anabuki, N. 2008, PASJ 60, 307
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Suzaku observations of early-type galaxies

  • K. Matsushita (a1), Y. Fukazawa (a2), K. Hayashi (a2), S. Konami (a1), R. Nagino (a1), T. Ohashi (a3), Y. Tawara (a4) and M. Tozuka (a1)...

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