III/121 Catalogue of stellar abundances (Marecki+ 1986)
Catalogue of stellar abundances
Marecki A., Strobel J., Strobel A.
<Torun Observatory (1986)>
=1994yCat.3121....0M 1994yCat.3121....0M
ADC_Keywords: Abundances, [Fe/H] ; Abundances, peculiar ;
Description:
The catalogue, compiled at the Torun Observatory, contains the
published abundances.
File Summary:
--------------------------------------------------------------------------------
FileName Lrecl Records Explanations
--------------------------------------------------------------------------------
ReadMe 80 . This file
catalog.dat 79 16716 The catalogue of abundances (1470 stars)
--------------------------------------------------------------------------------
Byte-per-byte Description of file: catalog.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 8 A8 --- Name Identification of the star (HD number)
10- 12 I3 --- Seq [1/212] Running number for a star
14- 16 A3 --- Ion Name of the element. M/H denotes metallicity
18 I1 --- A [1/5]? Code of the form of the original abundance
determination (1)
20- 25 A6 --- refEl Name of the reference element: H12 for log.H=12,
H24 for log.H=24, Fe, etc...)
27 A1 --- St [OSB] Code for the reference object, O=Sun (2)
29- 38 A10 --- Sname Name of the standard (reference) star or object
40 A1 --- n_Abun [HSPE] Method of abundance determination (3)
42- 48 A7 --- Abun Value of the abundance determination is
cited in the publication
50- 53 A4 --- e_Abun Error of the abundance determination
as cited in the publication
55- 60 A6 --- Ref Bibliographic reference (the list of references
is not available)
62- 79 A18 --- Com Comments
--------------------------------------------------------------------------------
Note (1): this code specifies how the abundance was given in the original
literature:
1 = (Nel/Nel) relative to the reference star
2 = log(Nel/Nel) relative to the reference star
3 = log(Nel) for log.H = 12 or log.H = 24
4 = (Nel/Nel)
5 = other form
Note (2): code for the reference object relative to which the abundance
is determined:
O = the Sun
S = the star other than the Sun
B = other reference "object" like average value of the abundance of
a given element for a group of stars
Note (3): code for the method of abundance determination as follows:
H = based on spectra of high (up to 20Å/mm) dispersion
S = based on spectra of small dispersion
P = based on photographic photometry
E = based on photoelectric photometry
--------------------------------------------------------------------------------
History:
* 09-Sep-1997: standardization by James E. Gass [SSDOO/ADC]
* 02-Apr-2016: cosmetic changes (names of columns, data alignments)
(End) [CDS] 26-Mar-1994