Issue |
A&A
Volume 501, Number 1, July I 2009
|
|
---|---|---|
Page(s) | 157 - 169 | |
Section | Extragalactic astronomy | |
DOI | https://doi.org/10.1051/0004-6361/200810978 | |
Published online | 29 April 2009 |
Gravitational potential and X-ray luminosities of early-type galaxies observed with XMM-Newton and Chandra
Tokyo University of Science, 1-3 Kagurazaka, Shinjyuku-ku, 162-8601 Tokyo, Japan e-mail: j1207705@ed.kagu.tus.ac.jp; matusita@rs.kagu.tus.ac.jp
Received:
17
September
2008
Accepted:
25
March
2009
Aims. We study the dark matter content in early-type galaxies and investigate whether X-ray luminosities of early-type galaxies are determined by the surrounding gravitational potential.
Methods. We derived gravitational mass profiles of 22 early-type galaxies observed with XMM-Newton and Chandra.
Results. Sixteen galaxies show constant or
decreasing radial temperature profiles, and their X-ray luminosities
are consistent with kinematical energy input from stellar mass
loss. The temperature profiles of the other 6 galaxies increase with
radius, and their X-ray luminosities are significantly higher.
The integrated mass-to-light ratio of each galaxy is constant at
that of stars within 0.5–, and increases with radius, where
re is the effective radius of a galaxy. The scatter of the central
mass-to-light ratio of galaxies was less in K-band light. At
, the
integrated mass-to-light ratios of galaxies with flat or decreasing
temperature profiles are twice the value at
, where the stellar
mass dominates, and at
, these increase to three times the value
at
.
Conclusions. This feature should reflect common dark and stellar mass distributions
in early-type galaxies: within , the mass of dark matter is similar
to the stellar mass, while within
, the former is larger than the
latter by a factor of two. In contrast, X-ray luminous galaxies have
higher gravitational mass in the outer regions than X-ray faint
galaxies. We describe these X-ray luminous galaxies as the central
objects of large potential structures; the presence or absence of this
potential is the main source of the large scatter in the X-ray
luminosity.
Key words: galaxies: elliptical and lenticular, cD / galaxies: ISM / X-rays: galaxies / X-rays: ISM
© ESO, 2009
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