- ... binaries
- Based on observations obtained with XMM-Newton, an ESA science
mission with instruments and contributions directly funded by
ESA Member States and the USA (NASA).
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ...1,
- Present address: Columbia Astrophysics Laboratory, Mailcode
5247, 550 West 120th Street, New York, NY 10027, USA.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ...2002)
- A safety check with more recent
calibration available with SAS 5.3.3 confirms that our results are robust. Note
that the C abundance may suffer from some bias since the shape of the EMdistribution below 1 MK cannot be constrained from the XMM-Newton data.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ...1995)
- [O/H] = -0.25, [Mg/H] = -0.10, [Si/H] = -0.30,
[Ca/H] = -0.20, [Fe/H] = -0.50, [Ni/H] = -0.40.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ...1994)
-
,
,
,
,
,
,
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.