- ...
list
- Tables 5, 6, 7 are also available in electronic form at
the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via
http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/373/63
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ... Paradijs
- Jan van Paradijs passed away on November 2nd, 1999.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ... accuracy
- As a concequence
of this data quality based decision variable sources are preferentially listed
in their luminous state which may have different spectral characteristics
compared with their less luminous state. Therefore sources detected as
variable (see Tables 2 and 3) are marked
with a "
''-sign in front of their RXJ-number.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ...1996)
- Kahabka (1999) used not only
but also
and
(with reference to the local
-value at the
source position) and their respective ratios to discriminate supersoft
sources. Using these criteria and the source list of S97, he came up with an
additional 26 new supersoft source candidates, 4 of them correlated with
foreground stars in S97 and 4 with supernova remnants. Excluding these 8
sources, 18 additional supersoft source candidates in M 31 remain.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.