2007MNRAS.382..553L

Query : 2007MNRAS.382..553L

2007MNRAS.382..553L - Mon. Not. R. Astron. Soc., 382, 553-566 (2007/December-1)

The abundances of nearby red clump giants.

LIU Y.J., ZHAO G., SHI J.R., PIETRZYNSKI G. and GIEREN W.

Abstract (from CDS):

Based on the analysis of high-resolution spectra with a high signal-to-noise ratio, we have determined the abundances of the α-elements O, Si, Ca and Ti, the iron peak elements V, Fe and Ni, and the heavy element Ba without the consideration of non-local thermodynamic equilibrium (NLTE) effect and the light neutron-rich elements Na, Mg and Al with an NLTE analysis for 63 nearby red clump giants. Fe abundances cover a logarithmic range between -0.60 and +0.35 relative to solar. All abundance ratios with respect to Fe are similar to those found in the Sun. Hyperfine structure (HFS) was taken into account when calculating V lines. The difference in abundances obtained with and without HFS can be as large as 0.5 dex.

Abstract Copyright: 2007 The Authors. Journal compilation © 2007 RAS

Journal keyword(s): stars: abundances - stars: atmospheres - stars: late-type

VizieR on-line data: <Available at CDS (J/MNRAS/382/553): table1.dat table2.dat table3.dat table4.dat table7.dat table8.dat table9.dat>

Simbad objects: 65

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Number of rows : 65
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 HD 360 HB* 00 08 17.5324307736 -08 49 26.801843988   7.014 5.980     K1II 57 0
2 HD 770 PM* 00 11 56.0565656472 -42 10 19.706103732   7.59 6.53     K0III 29 0
3 HD 3750 HB* 00 39 51.9501192576 -44 47 46.651236396   7.141 5.998     K1IIICNII 43 0
4 * phi01 Cet PM* 00 44 11.4000904231 -10 36 34.382643011   5.773 4.767     K0III 123 0
5 * lam02 Scl PM* 00 44 12.0990327144 -38 25 18.054207912   7.06 5.96     K1III 57 0
6 * 21 Cet PM* 00 54 17.5927919832 -08 44 26.390035212   7.086 6.161     G8III 90 0
7 * phi04 Cet HB* 00 58 43.8680525208 -11 22 47.910692424   6.566 5.614     G8III 81 0
8 HD 6559 PM* 01 06 07.7141953080 -23 59 32.943888024   7.180 6.114     K1III 51 0
9 * 32 Cet * 01 10 11.9457318744 -08 54 22.084762140   7.420 6.394     K0III 43 0
10 HD 8651 * 01 24 40.7865339576 -41 29 33.164287944   6.443 5.417     K0III 61 0
11 * del Phe PM* 01 31 15.1040942588 -49 04 21.730128530   4.918 3.935     G8.5IIIb 135 0
12 HD 10042 PM* 01 33 39.1710859344 -78 30 17.351232264   7.077 6.103     K0III 41 0
13 HD 10142 PM* 01 38 27.4839019872 -36 31 41.700679932   6.991 5.939     K0III 56 0
14 * pi. Scl PM* 01 42 08.6293373664 -32 19 37.155166068   6.287 5.256     K1II/III 61 0
15 HD 11643 PM* 01 53 23.1726086160 -38 35 40.673979852   7.234 6.086     K1/2III 38 0
16 HD 15471 * 02 28 35.4330784248 -31 06 08.812525068   7.216 6.105     K2IIICNII 35 0
17 * 75 Cet HB* 02 32 09.4224095904 -01 02 05.616571164   6.366 5.358 10.0   K1III 95 1
18 * iot Eri PM* 02 40 40.0348498136 -39 51 19.355490088   5.114 4.116     K0IIIb 100 0
19 HD 16975 * 02 42 06.6072699192 -38 23 01.273215804   6.909 5.988     G8III 44 0
20 * bet For RG* 02 49 05.4189042528 -32 24 21.232006884 6.14 5.45 4.46 3.70 3.16 G9IIIb 89 0
21 * tau02 Eri PM* 02 51 02.3271116481 -21 00 14.441517124 6.28 5.67 4.77 4.07 3.60 K0III 99 0
22 HD 24706 SB* 03 53 33.3431392008 -46 53 37.265782632   7.164 5.921     K2III 66 0
23 HD 25170 PM* 03 56 03.9962013072 -63 27 49.373859060   7.240 6.137     K1/2III 32 0
24 * alf Hor PM* 04 14 00.1142226166 -42 17 39.726755131 5.97 4.96 3.86 3.00 2.41 K2III 150 0
25 Cl Melotte 25 OpC 04 30 27.4 +16 46 43           ~ 3309 0
26 * 89 Vir PM* 13 49 52.2828951024 -18 08 03.009309756   6.018 4.959     K0+IIIb 116 0
27 HD 139254 HB* 15 37 48.0415231272 -23 08 30.145550532   6.854 5.790     K0III 51 0
28 HD 138289 PM* 15 39 18.3971214240 -77 55 04.819554696   7.431 6.181     K2.5IIIbCN1.5Ba+0.5 45 0
29 * alf Ser PM* 15 44 16.0741095811 +06 25 32.268792881 5.080 3.800 2.630 1.82 1.25 K2IIIbCN1 533 0
30 * ome Ser PM* 15 50 17.5468226304 +02 11 47.432004216   6.236 5.217     K0IV 146 1
31 * tet Lib PM* 15 53 49.5379222294 -16 43 45.469368699 5.99 5.17 4.16 3.44 2.92 G9IIIb 124 0
32 * eta Nor * 16 03 12.8974905224 -49 13 46.905295622   5.569 4.643     G8III 43 0
33 HD 143787 PM* 16 03 20.6231448768 -25 51 54.873258444   6.202 4.966     K3III 53 0
34 * 43 Ser * 16 03 45.6910511280 +04 59 12.595656228   7.036 6.068     G9III 49 0
35 * 16 Her PM* 16 15 28.6349735016 +18 48 29.117594304 7.82 6.81 5.69     K3III 67 0
36 * eps Oph PM* 16 18 19.2902245358 -04 41 33.047349888 4.95 4.21 3.23 2.54 2.05 G9.5IIIbFe-0.5 246 0
37 * gam02 Nor PM* 16 19 50.4223079953 -50 09 19.821590813 6.27 5.10 4.02 3.24 2.66 K0III 78 0
38 * psi Oph PM* 16 24 06.1777460190 -20 02 14.352188619 6.37 5.53 4.50 3.72 3.22 K0-II-III 91 0
39 * bet Aps PM* 16 43 04.6585772236 -77 31 02.759334193   5.30 4.24     K0III 55 0
40 * Q Sco PM* 17 36 32.8551435432 -38 38 06.891848556   5.357 4.267     G8/K0III/IV 47 0
41 HD 160315 PM* 17 39 08.5045924128 +02 01 40.979804268   7.273 6.253     K0III 63 0
42 * 1 Sgr * 18 11 43.3327588368 -23 42 04.433754384   6.03 4.98     K0III 44 0
43 HD 167768 PM* 18 16 53.1010153824 -03 00 26.647248600   6.89 6.00     G8III 108 0
44 * lam Sgr PM* 18 27 58.2407185 -25 25 18.114589 4.75 3.85 2.81 2.06 1.50 K1IIIb 290 0
45 * zet Tel PM* 18 28 49.8593702175 -49 04 14.117954578   5.12 4.11     K1III-IV 59 0
46 HD 176704 PM* 19 02 27.6750403056 -24 50 48.571522440   6.849 5.628     K2III 52 0
47 * omi Sgr PM* 19 04 40.9820400284 -21 44 29.385451232 5.63 4.77 3.77 3.05 2.52 G9IIIb 111 0
48 * del CrA PM* 19 08 20.9696916432 -40 29 48.112728468   5.664 4.571     K1III 37 0
49 HD 189561 RG* 20 01 23.8467090408 -22 44 14.312051448   6.982 5.999     K0III 39 0
50 * mu.02 Pav PM* 20 01 52.4617617696 -66 56 38.271651288   6.546 5.331     K2IVCNII 43 0
51 HD 191584 PM* 20 12 23.8401127176 -42 46 48.215657604   7.440 6.191     K1III 41 0
52 * alf Ind PM* 20 37 34.0321723878 -47 17 29.405217299 4.90 4.11 3.11     K0III-IV 141 0
53 * b Cap PM* 21 28 43.4007028168 -21 48 25.847136535 6.00 5.40 4.50 3.83 3.37 G7IIIbFe-1 86 0
54 HD 214122 PM* 22 36 35.4401305824 -31 39 49.646890872   6.903 5.808     K2III 28 0
55 * rho Gru PM* 22 43 29.9762552808 -41 24 51.643891310   5.854 4.835     K0III 81 0
56 * del PsA * 22 55 56.9001952776 -32 32 22.646172516   5.172 4.208     G8III 67 0
57 * psi01 Aqr PM* 23 15 53.4940495770 -09 05 15.844964053 6.37 5.36 4.25 3.46 2.90 K1-IIIFe-0.5 260 1
58 * gam Psc PM* 23 17 09.9371132484 +03 16 56.245688417 5.20 4.62 3.70 2.98 2.47 G9III:Fe-2 277 0
59 * gam Scl PM* 23 18 49.4375987895 -32 31 55.278901051   5.528 4.406     K1III 90 0
60 HD 220572 HB* 23 25 19.4647706184 -56 50 56.341542084   6.661 5.597     K0III 49 0
61 * tet Psc PM* 23 27 58.0946643849 +06 22 44.372303191 6.41 5.38 4.30 3.50 2.97 K0.5III 185 0
62 * 70 Peg SB* 23 29 09.2992398120 +12 45 37.979571348 6.24 5.50 4.56 3.82 3.37 G8IIIa 159 0
63 HD 222493 PM* 23 41 08.9122868619 -11 40 50.345125880   6.92 5.92     K0III 50 0
64 * 20 Psc PM* 23 47 56.5419212784 -02 45 41.752306188   6.433 5.490     K0III 99 0
65 NAME Galactic Bulge reg ~ ~           ~ 4794 0

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