2010ApJ...714.1001S


Query : 2010ApJ...714.1001S

2010ApJ...714.1001S - Astrophys. J., 714, 1001-1014 (2010/May-2)

Abundances of C, N, sr, and ba on the red giant branch of ω Centauri.

STANFORD L.M., DA COSTA G.S. and NORRIS J.E.

Abstract (from CDS):

Abundances relative to iron for carbon, nitrogen, strontium, and barium are presented for 33 stars on the red giant branch (RGB) of the globular cluster ω Centauri. They are based on intermediate-resolution spectroscopic data covering the blue spectral region analyzed using spectrum synthesis techniques. The data reveal the existence of a broad range in the abundances of these elements, and a comparison with similar data for main-sequence stars enables insight into the evolutionary history of the cluster. The majority of the RGB stars were found to be depleted in carbon, i.e., [C/Fe] < 0, while [N/Fe] for the same stars shows a range of ∼1 dex, from [N/Fe] ≈ 0.7 to 1.7 dex. The strontium-to-iron abundance ratios varied from solar to mildly enhanced (0.0 ≤ [Sr/Fe] ≤ 0.8), with [Ba/Fe] generally equal to or greater than [Sr/Fe]. The carbon and nitrogen abundance ratios for the one known CH star in the sample, ROA 279, are [C/Fe] = 0.6 and [N/Fe] = 0.5 dex. Evidence for evolutionary mixing on the RGB is found from the fact that the relative carbon abundances on the main sequence are generally higher than those on the RGB. However, comparison of the RGB and main-sequence samples shows that the upper level of nitrogen enhancement is similar in both sets at [N/Fe] ≈ 2.0 dex. This is most likely the result of primordial rather than evolutionary mixing processes. One RGB star, ROA 276, was found to have Sr and Ba abundance ratios similar to the anomalous Sr-rich main-sequence star S2015448. High-resolution spectra of ROA 276 were obtained with the Magellan Telescope/MIKE spectrograph combination to confirm this result, revealing that ROA 276 is indeed an unusual star. For this star, calculations of the depletion effect, the potential change in surface abundance that results from the increased depth of the convective envelope as a star moves from the main sequence to the RGB, strongly suggest that the observed Sr enhancement in ROA 276 is of primordial origin, rather than originating from a surface accretion event.

Abstract Copyright: ∼

Journal keyword(s): globular clusters: general - globular clusters: individual: ω Centauri

Simbad objects: 53

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Number of rows : 53
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 NGC 104 GlC 00 24 05.359 -72 04 53.20     4.09     ~ 4158 0
2 Cl* NGC 5139 SDN 2015448 * 13 24 49.1227400304 -47 40 34.771139868   18.91 18.22     ~ 5 0
3 NGC 5139 253 RG* 13 25 06.7227395856 -47 26 52.769765148   13.73 12.25     ~ 36 0
4 NGC 5139 159 RG* 13 25 17.5229869368 -47 24 26.555561460   13.369 12.004 11.704 10.45 ~ 45 0
5 NGC 5139 53 RG* 13 25 21.3164617824 -47 36 54.201274884   13.263 11.548 11.074   ~ 43 0
6 NGC 5139 43 RG* 13 25 39.5070925320 -47 14 05.509636440   13.25 11.42     ~ 35 0
7 2MASS J13254217-4733437 RG* 13 25 42.1720570392 -47 33 43.801448904 16.41 14.770 13.358   12.005 ~ 19 0
8 NGC 5139 171 RG* 13 25 45.1479161160 -47 32 38.295786444 14.94     11.645 10.519 ~ 35 0
9 NGC 5139 447 RB? 13 25 46.3328043792 -47 25 59.677976460   14.45 12.74   10.874 S 22 0
10 NGC 5139 94 RG* 13 25 51.2071380912 -47 27 01.754511732 14.24 13.083 11.701 11.364   ~ 36 0
11 NGC 5139 252 RG* 13 25 51.3418441968 -47 16 40.016073720   13.430 12.229     ~ 27 0
12 2MASS J13255200-4730163 AB* 13 25 52.0014791520 -47 30 16.405388712 14.21   11.350 11.004   ~ 49 0
13 SOPS IV e-94 C* 13 26 01.5892714032 -47 33 05.967491724   13.184 11.444 11.072 9.966 C1,3p 58 0
14 2MASS J13260383-4728327 RG* 13 26 03.8375820552 -47 28 32.726583984   14.950 13.789   12.408 ~ 14 0
15 2MASS J13261094-4725444 RG* 13 26 10.9370938224 -47 25 44.495248764   12.86 11.54     ~ 36 0
16 2MASS J13261120-4728435 RG* 13 26 11.2122788208 -47 28 43.621679532   13.98 12.50     ~ 33 0
17 2MASS J13261954-4716345 RG* 13 26 19.5473955312 -47 16 34.505962392   13.32 12.15     ~ 48 0
18 NGC 5139 150 RG* 13 26 23.6649086064 -47 42 42.409293624   13.692 11.946 11.588   ~ 40 0
19 NGC 5139 201 RG* 13 26 24.9957849312 -47 27 06.449465988   13.961 12.262     S 32 0
20 2MASS J13262921-4731092 RG* 13 26 29.2177769400 -47 31 09.238524528   14.311 12.443   10.889 S 25 0
21 2MASS J13263222-4730564 RG* 13 26 32.2363006632 -47 30 56.461118616   14.486 12.847   11.437 ~ 7 0
22 2MASS J13263410-4726212 RG* 13 26 34.1143119768 -47 26 21.173393832   14.263 12.077   10.844 ~ 13 0
23 NGC 5139 74 RG* 13 26 34.5299238720 -47 20 05.450209548   13.05 11.61     ~ 44 0
24 2MASS J13263483-4734110 RG* 13 26 34.8426950352 -47 34 11.125321320 16.056 14.039 12.249 11.306 10.498 ~ 35 0
25 2MASS J13264077-4736435 RG* 13 26 40.7721809832 -47 36 43.635788280   14.580 13.105   11.809 ~ 13 0
26 Cl* NGC 5139 WFI 230189 * 13 26 44.8509742872 -47 29 04.300068732   14.595     11.747 ~ 2 0
27 NGC 5139 480 RB? 13 26 47.2375070808 -47 34 12.317843964   14.196 12.923   11.655 ~ 27 0
28 NGC 5139 GlC 13 26 47.28 -47 28 46.1           ~ 3677 0
29 2MASS J13265070-4721066 RG* 13 26 50.7102780528 -47 21 06.755761080   14.970 13.675   12.382 ~ 13 0
30 2MASS J13265071-4737010 RG* 13 26 50.7174210264 -47 37 01.158926736   14.28 12.71   11.159 K5 51 0
31 2MASS J13265076-4733038 RG* 13 26 50.7729103008 -47 33 03.857447520   13.83 12.31   11.037 ~ 21 0
32 Cl* NGC 5139 SDN 8001811 * 13 26 52.1073908640 -47 11 47.921382744   18.420 17.800     ~ 3 0
33 NGC 5139 84 RG* 13 26 55.0638382872 -47 22 27.179341824 15.46 13.44 11.93   10.077 ~ 40 0
34 2MASS J13265554-4734234 RG* 13 26 55.5524112504 -47 34 23.415322584 15.133 13.57 11.83 10.945 10.006 K4: 42 0
35 2MASS J13265674-4720527 RG* 13 26 56.7434661744 -47 20 52.749110904 14.90 13.08 11.61   9.923 ~ 33 0
36 NGC 5139 336 RB? 13 26 58.222 -47 25 45.82   14.177 12.808     ~ 9 0
37 NGC 5139 517 RB? 13 27 05.4717788856 -47 24 37.016838612   14.511 13.030   11.555 K5: 18 0
38 Cl* NGC 5139 LEID 33139 RG* 13 27 06.9223203000 -47 24 23.407434468   14.880 13.645   12.289 ~ 14 0
39 2MASS J13270904-4723384 RG* 13 27 09.0515161128 -47 23 38.309059284 15.02 13.11 11.89     ~ 37 0
40 NGC 5139 58 RG* 13 27 09.6100609776 -47 20 51.403712712 14.27 13.097 11.625 11.256   ~ 52 0
41 2MASS J13271206-4729449 RG* 13 27 12.0775859232 -47 29 44.922617484 14.89 13.140 11.645     ~ 27 0
42 Cl* NGC 5139 LEID 32149 * 13 27 14.5543893600 -47 23 51.132283620   14.870 13.568 13.46 12.111 ~ 12 0
43 NGC 5139 477 Pe* 13 27 15.7162460208 -47 26 02.233002624   13.953 12.883     ~ 8 0
44 Cl* NGC 5139 SDN 7007334 * 13 27 17.4517483728 -47 07 29.599813812   18.970 18.440     ~ 3 0
45 2MASS J13272355-4728072 RG* 13 27 23.5657140960 -47 28 07.200070536 15.68 13.93 12.17   10.226 ~ 34 0
46 NGC 5139 139 RG* 13 27 28.8888033336 -47 21 39.321445464   13.42 11.90   10.377 ~ 36 0
47 2MASS J13273303-4726120 RG* 13 27 33.0466654440 -47 26 11.965454232 16.01 14.050 12.512   10.935 ~ 27 0
48 NGC 5139 219 RG* 13 28 13.5721791960 -47 24 23.564480436   13.802 12.165 11.825   ~ 41 0
49 Cl* NGC 5139 SDN 9005309 * 13 28 14.3374063344 -47 45 33.354384588   18.830 18.290     ~ 3 0
50 NGC 5139 279 RG* 13 28 21.2929487544 -47 20 30.256651860   12.8 12.32 12.14 11.04 ~ 28 0
51 Cl* NGC 5139 SDN 5004811 * 13 28 44.6921530416 -47 31 06.583757628   18.170 17.490     ~ 3 0
52 M 13 GlC 16 41 41.634 +36 27 40.75     5.8     ~ 2291 0
53 NGC 5139 425 * ~ ~   14.37 12.68     S 15 0

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