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J/ApJS/99/637 Equivalent widths for 54 red giants (Norris+ 1995)
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Equivalent widths for 54 red giants in 47 Tucanae, Omega Centauri, NGC 6397,
M22, and NGC 6752
Norris J.E., Da Costa G.S., Tingay S.J.
<Astrophys. J. Suppl. Ser. 99, 637 (1995)>
=1995ApJS...99..637N
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ADC_Keywords: Stars, giant ; Equivalent widths ; Clusters, globular
Keywords: globular clusters: general - stars: abundances - stars: late-type
Abstract:
We present equivalent widths for 54 red giants in five globular
clusters, and compare the data with those of other workers. This
material will form the basis for subsequent analyses of the chemical
inhomogeneity of Omega Cen and M22.
Objects:
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RA (2000) DE Designation(s)
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14 15 43.5 +19 12 37 Alpha Boo = HD 124897 = HR 5340
13 26 46 -47 28.6 Omega Cen = = HD 116790 = NGC 5139
00 23 22 -72 04.4 47 Tuc = NGC 104
18 36.4 -23 55 M 22 = NGC 6656
19 10.8 -59 59 NGC 6752
17 40.9 -53 41 NGC 6397
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File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table1 117 361 *Equivalent widths (mA) and atomic data for
Alpha Bootis and Omega Centauri giants
table2 117 361 *Equivalent widths (mA) and atomic data for
Omega Centauri giants
table3 109 361 *Equivalent widths (mA) for 47 Tucanae, NGC 6397,
M22, and NGC 6752 giants
table.tex 45 11 AASTeX main file for formatting tables
table1.tex 144 807 AASTeX version of table1
table2.tex 140 807 AASTeX version of table2
table3.tex 155 807 AASTeX version of table3
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Note on table1 and table2: The nomenclature is from Woolley et al.
(1966ROAn....2....1W)
Note on table3: The nomenclature is from Lee (1977A&AS...27..381L) for 47 Tuc;
Woolley et al. (1961RGOB...43..303W) for NGC 6397;
Arp & Melbourne (1959AJ.....64...28A) for M 22;
Alcaino (1972A&A....16..220A), Cannon & Stobie (1973MNRAS.162..227C) and
Cannon & Leee (priv. comm.) for NGC 6752
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Byte-by-byte Description of file: table1
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Bytes Format Units Label Explanations
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1- 7 A7 --- Species Atomic species
8- 14 F7.2 0.1nm Lambda Spectral line wavelength
16- 20 F5.2 --- Chi Chi value
22- 26 F5.2 --- gf *[]? Log gf value
30- 32 I3 10-4nm AlpBoo []? Equivalent width for Alpha Boo
34 A1 --- l_EW40 *[<b] Limiting character for EW40
35- 37 I3 10-4nm EW40 *[]? Equivalent width for Ome Cen star 40
39 A1 --- l_EW42 [<b] Limiting character for EW42
40- 42 I3 10-4nm EW42 []? Equivalent width for Ome Cen star 42
44 A1 --- l_EW43 [<b] Limiting character for EW43
45- 47 I3 10-4nm EW43 []? Equivalent width for Ome Cen star 43
49 A1 --- l_EW46 [<b] Limiting character for EW46
50- 52 I3 10-4nm EW46 []? Equivalent width for Ome Cen star 46
54 A1 --- l_EW48 [<b] Limiting character for EW48
55- 57 I3 10-4nm EW48 []? Equivalent width for Ome Cen star 48
59 A1 --- l_EW53 [<b] Limiting character for EW53
60- 62 I3 10-4nm EW53 []? Equivalent width for Ome Cen star 53
64 A1 --- l_EW58 [<b] Limiting character for EW58
65- 67 I3 10-4nm EW58 []? Equivalent width for Ome Cen star 58
69 A1 --- l_EW74 [<b] Limiting character for EW74
70- 72 I3 10-4nm EW74 []? Equivalent width for Ome Cen star 74
74 A1 --- l_EW84 [<b] Limiting character for EW84
75- 77 I3 10-4nm EW84 []? Equivalent width for Ome Cen star 84
79 A1 --- l_EW94 [<b] Limiting character for EW94
80- 82 I3 10-4nm EW94 []? Equivalent width for Ome Cen star 94
84 A1 --- l_EW100 [<b] Limiting character for EW100
85- 87 I3 10-4nm EW100 []? Equivalent width for Ome Cen star 100
89 A1 --- l_EW102 [<b] Limiting character for EW102
90- 92 I3 10-4nm EW102 []? Equivalent width for Ome Cen star 102
94 A1 --- l_EW132 [<b] Limiting character for EW132
95- 97 I3 10-4nm EW132 []? Equivalent width for Ome Cen star 132
99 A1 --- l_EW144 [<b] Limiting character for EW144
100-102 I3 10-4nm EW144 []? Equivalent width for Ome Cen star 144
104 A1 --- l_EW150 [<b] Limiting character for EW150
105-107 I3 10-4nm EW150 []? Equivalent width for Ome Cen star 150
109 A1 --- l_EW155 [<b] Limiting character for EW155
110-112 I3 10-4nm EW155 []? Equivalent width for Ome Cen star 155
114 A1 --- l_EW159 [<b] Limiting character for EW159
115-117 I3 10-4nm EW159 []? Equivalent width for Ome Cen star 159
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Note on gf:
Log gf value based on an inverted model atmosphere analysis of the
line strengths for Alpha Boo of those lines which are used to
determine abundances.
Note on l_EW40:
The limiting characters for EW40 and all other equivalent width
fields are: '<' if the EW is an upper limit; 'b' if the line
appeared to be a blend or to have a profile which is not conducive
to line strength measurement.
Note on EW40:
For EW40 and all other equivalent width fields, no data value is
given in the case of a blend (see the comment for l_EW40) or when no
attempt was made to measure the line (usually because it fell outside
the detector, fell in a proscribed wavelength range, or was
contaminated by terrestrial water vapor).
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Byte-by-byte Description of file: table2
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Bytes Format Units Label Explanations
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1- 7 A7 --- Species Atomic species
8- 14 F7.2 0.1nm Lambda Spectral line wavelength
16- 20 F5.2 --- Chi Chi value
22- 26 F5.2 --- gf *[]? Log gf value
29 A1 --- l_EW161 *[<b] Limiting character for EW161
30- 32 I3 10-4nm EW161 []? Equivalent width for Ome Cen star 161
34 A1 --- l_EW162 *[<b] Limiting character for EW162
35- 37 I3 10-4nm EW162 *[]? Equivalent width for Ome Cen star 162
39 A1 --- l_EW171 [<b] Limiting character for EW171
40- 42 I3 10-4nm EW171 []? Equivalent width for Ome Cen star 171
44 A1 --- l_EW179 [<b] Limiting character for EW179
45- 47 I3 10-4nm EW179 []? Equivalent width for Ome Cen star 179
49 A1 --- l_EW182 [<b] Limiting character for EW182
50- 52 I3 10-4nm EW182 []? Equivalent width for Ome Cen star 182
54 A1 --- l_EW201 [<b] Limiting character for EW201
55- 57 I3 10-4nm EW201 []? Equivalent width for Ome Cen star 201
59 A1 --- l_EW213 [<b] Limiting character for EW213
60- 62 I3 10-4nm EW213 []? Equivalent width for Ome Cen star 213
64 A1 --- l_EW219 [<b] Limiting character for EW219
65- 67 I3 10-4nm EW219 []? Equivalent width for Ome Cen star 219
69 A1 --- l_EW231 [<b] Limiting character for EW231
70- 72 I3 10-4nm EW231 []? Equivalent width for Ome Cen star 231
74 A1 --- l_EW234 [<b] Limiting character for EW234
75- 77 I3 10-4nm EW234 []? Equivalent width for Ome Cen star 234
79 A1 --- l_EW248 [<b] Limiting character for EW248
80- 82 I3 10-4nm EW248 []? Equivalent width for Ome Cen star 248
84 A1 --- l_EW252 [<b] Limiting character for EW252
85- 87 I3 10-4nm EW252 []? Equivalent width for Ome Cen star 252
89 A1 --- l_EW253 [<b] Limiting character for EW253
90- 92 I3 10-4nm EW253 []? Equivalent width for Ome Cen star 253
94 A1 --- l_EW279 [<b] Limiting character for EW279
95- 97 I3 10-4nm EW279 []? Equivalent width for Ome Cen star 279
99 A1 --- l_EW287 [<b] Limiting character for EW287
100-102 I3 10-4nm EW287 []? Equivalent width for Ome Cen star 287
104 A1 --- l_EW357 [<b] Limiting character for EW357
105-107 I3 10-4nm EW357 []? Equivalent width for Ome Cen star 357
109 A1 --- l_EW371 [<b] Limiting character for EW371
110-112 I3 10-4nm EW371 []? Equivalent width for Ome Cen star 371
114 A1 --- l_EW480 [<b] Limiting character for EW480
115-117 I3 10-4nm EW480 []? Equivalent width for Ome Cen star 480
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Note on gf:
Log gf value based on an inverted model atmosphere analysis of the
line strengths for Alpha Boo of those lines which are used to
determine abundances.
Note on l_EW161, l_EW162:
The limiting characters for EW161 and all other equivalent width
fields are: '<' if the EW is an upper limit; 'b' if the line
appeared to be a blend or to have a profile which is not conducive
to line strength measurement.
Note on EW161, EW162:
For EW161 and all other equivalent width fields, no data value is
given in the case of a blend (see the comment for l_EW161) or when no
attempt was made to measure the line (usually because it fell outside
the detector, fell in a proscribed wavelength range, or was
contaminated by terrestrial water vapor).
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Byte-by-byte Description of file: table3
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Bytes Format Units Label Explanations
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1- 7 A7 --- Species Atomic species
8- 14 F7.2 0.1nm Lambda Spectral line wavelength
16 A1 --- l_L5529 *[<b] Limiting character for L5529
17- 19 I3 --- L5529 *[]? EW for 47 Tuc object L5529
21 A1 --- l_R211 [<b] Limiting character for R211
22- 24 I3 10-4nm R211 []? EW for NGC 6397 object R211
26 A1 --- l_R469 [<b] Limiting character for R469
27- 29 I3 10-4nm R469 []? EW for NGC 6397 object R469
31 A1 --- l_I12 [<b] Limiting character for I12
32- 34 I3 10-4nm I12 []? EW for M22 object I-12
36 A1 --- l_I57 [<b] Limiting character for I57
37- 39 I3 10-4nm I57 []? EW for M22 object I-57
41 A1 --- l_I86 [<b] Limiting character for I86
42- 44 I3 10-4nm I86 []? EW for M22 object I-86
46 A1 --- l_III12 [<b] Limiting character for III12
47- 49 I3 10-4nm III12 []? EW for M22 object III-12
51 A1 --- l_III14 [<b] Limiting character for III14
52- 54 I3 10-4nm III14 []? EW for M22 object III-14
56 A1 --- l_III96 [<b] Limiting character for III96
57- 59 I3 10-4nm III96 []? EW for M22 object III-96
61 A1 --- l_IV20 [<b] Limiting character for IV20
62- 64 I3 10-4nm IV20 []? EW for M22 object IV-20
66 A1 --- l_IV76 [<b] Limiting character for IV76
67- 69 I3 10-4nm IV76 []? EW for M22 object IV-76
71 A1 --- l_IV88 [<b] Limiting character for IV88
72- 74 I3 10-4nm IV88 []? EW for M22 object IV-88
76 A1 --- l_IV102 [<b] Limiting character for IV102
77- 79 I3 10-4nm IV102 []? EW for M22 object IV-102
81 A1 --- l_A29 [<b] Limiting character for A29
82- 84 I3 10-4nm A29 []? EW for NGC 6752 object A29
86 A1 --- l_A45 [<b] Limiting character for A45
87- 89 I3 10-4nm A45 []? EW for NGC 6752 object A45
91 A1 --- l_CS3 [<b] Limiting character for CS3
92- 94 I3 10-4nm CS3 []? EW for NGC 6752 object CS3
96 A1 --- l_C1015 [<b] Limiting character for C1015
97- 99 I3 10-4nm C1015 []? EW for NGC 6752 object C1015
101 A1 --- l_C1066 [<b] Limiting character for C1066
102-104 I3 10-4nm C1066 []? EW for NGC 6752 object C1066
106 A1 --- l_C1089 [<b] Limiting character for C1089
107-109 I3 10-4nm C1089 []? EW for NGC 6752 object C1089
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Note on l_L5529:
The limiting characters for L5529 and all other equivalent width
fields are: '<' if the EW is an upper limit; 'b' if the line
appeared to be a blend or to have a profile which is not conducive
to line strength measurement.
Note on L5529:
For L5529 and all other equivalent width fields, no data value is
given in the case of a blend (see the comment for l_L5529) or when no
attempt was made to measure the line (usually because it fell outside
the detector, fell in a proscribed wavelength range, or was
contaminated by terrestrial water vapor).
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Origin: AAS CD-ROM series, Volume 5, 1995 Lee Brotzman [ADS] 31-Aug-1995
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(End) [CDS] 02-Feb-1996