Astronomy and Astrophysics – Astrophysics
Scientific paper
1996-09-06
Astronomy and Astrophysics
Astrophysics
39 pages, TeX file, 5 figures, Accepted for publication in the ApJ
Scientific paper
10.1086/303684
We present estimates for the iron content of the stellar and diffused components of elliptical galaxies, as derived respectively from integrated optical spectra and from ASCA X-ray observations. A macroscopic discrepancy emerges between the expected iron abundances in the hot interstellar medium (ISM) and what is indicated by the X-ray observations, especially when allowance is made for the current iron enrichment by Type Ia supernovae. This strong discrepancy, that in some extreme instances may be as large as a factor of $\sim 20$, calls into question our current understanding of supernova enrichment and chemical evolution of galaxies. We discuss several astrophysical implications of the inferred low iron abundances in the ISM, including the chemical evolution of galaxies and cluster of galaxies, the evolution of gas flows in ellipticals, and the heating of the intracluster medium. Some of the consequences appear hard to accept, and in the attempt to avoid some of these difficulties we explore ways of hiding or diluting iron in the ISM of ellipticals. None of these possibilities appears astrophysically plausible, and we alternatively rise the question of the reliability of iron-L line diagonostic tools. Various thin plasma emission models are shown to give iron abundances that may differ significantly, especially at low temperatures ($kT \lsim 1$ keV). From a collection of ASCA and other X-ray observatory data, it is shown that current thin plasma codes tend to give very low iron abundances when the temperature of the objects is below $\sim 1$ keV. We conclude that -- besides rethinking the chemical evolution of galaxies -- one should also consider the possibility that existing thin plasma models may incorporate inaccurate atomic physics for the ions responsible for the iron-L complex.
Arimoto Nobuo
Ishimaru Yuhri
Matsushita Kyoko
Ohashi Takaya
Renzini Alvio
No associations
LandOfFree
The Iron Discrepancy in Elliptical Galaxies after ASCA does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The Iron Discrepancy in Elliptical Galaxies after ASCA, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Iron Discrepancy in Elliptical Galaxies after ASCA will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-382275