All Tables
- Table 2:
Atomic data for the 1.046
m S I triplet.
Column 5 lists the equivalent width in the spectrum of
G 29-23 and the last column gives the derived
LTE sulphur abundance.
- Table 1:
Derived stellar parameters and abundances of sulphur and zinc.
LTE sulphur abundances are given for each of the three S I lines. The LTE Zn abundance is
the average of the values derived from the
Zn I lines.
In calculating [S/Fe] and [Zn/Fe], solar abundances log
= 7.50, log
= 7.20
and log
= 4.60 have been adopted. The non-LTE values of [S/Fe] and [Zn/Fe] are
based on the non-LTE corrections calculated by Takeda et al. (2005) for
a hydrogen collisional parameter
.
- Table A.1:
List of spectral lines and equivalent widths measured
in the UVES 2004 spectra of the following twelve stars:
(1) CD
,
(2) CD
,
(3) CS 22943-095,
(4) G 04-37,
(5) G 48-29,
(6) G 59-27,
(7) G 126-52,
(8) G 166-54,
(9) HD 84937,
(10) HD 338529,
(11) LP 635-14,
(12) LP 651-4.
- Table B.1:
V and
magnitudes, Strömgren indices, and
photometric and spectroscopic indices of the strength of the H
line.
The derived interstellar reddening of (
is given in Col. 10, and the absolute
visual magnitude derived from the Strömgren photometry is given in Col. 11.
Columns 12 and 13 give the absolute visual magnitude and its 1-
error derived from the
Hipparcos parallax if available with an error less than 30%.
- Table C.1:
S and Zn abundance measurements in DLAs.