2022A&A...668A.168C


Query : 2022A&A...668A.168C

2022A&A...668A.168C - Astronomy and Astrophysics, volume 668A168 (2022/12-1)

MINCE I. Presentation of the project and of the first year sample,.

CESCUTTI G., BONIFACIO P., CAFFAU E., MONACO L., FRANCHINI M., LOMBARDO L., MATAS PINTO A.M., LUCERTINI F., FRANCOIS P., SPITONI E., LALLEMENT R., SBORDONE L., MUCCIARELLI A., SPITE M., HANSEN C.J., DI MARCANTONIO P., KUCINSKAS A., DOBROVOLSKAS V., KORN A.J., VALENTINI M., MAGRINI L., CRISTALLO S. and MATTEUCCI F.

Abstract (from CDS):

Context. In recent years, Galactic archaeology has become a particularly vibrant field of astronomy, with its main focus set on the oldest stars of our Galaxy. In most cases, these stars have been identified as the most metal-poor. However, the struggle to find these ancient fossils has produced an important bias in the observations - in particular, the intermediate metal-poor stars (-2.5 < [Fe/H] < -1.5) have been frequently overlooked. The missing information has consequences for the precise study of the chemical enrichment of our Galaxy, in particular for what concerns neutron capture elements and it will be only partially covered by future multi object spectroscopic surveys such as WEAVE and 4MOST. Aims. Measuring at Intermediate Metallicity Neutron Capture Elements (MINCE) is gathering the first high-quality spectra (high signal-to-noise ratio, S/N, and high resolution) for several hundreds of bright and metal-poor stars, mainly located in our Galactic halo. Methods. We compiled our selection mainly on the basis of Gaia data and determined the stellar atmospheres of our sample and the chemical abundances of each star. Results. In this paper, we present the first sample of 59 spectra of 46 stars. We measured the radial velocities and computed the Galactic orbits for all stars. We found that 8 stars belong to the thin disc, 15 to disrupted satellites, and the remaining cannot be associated to the mentioned structures, and we call them halo stars. For 33 of these stars, we provide abundances for the elements up to zinc. We also show the chemical evolution results for eleven chemical elements, based on recent models. Conclusions. Our observational strategy of using multiple telescopes and spectrographs to acquire high S/N and high-resolution spectra for intermediate-metallicity stars has proven to be very efficient, since the present sample was acquired over only about one year of observations. Finally, our target selection strategy, after an initial adjustment, proved satisfactory for our purposes.

Abstract Copyright: © G. Cescutti et al. 2022

Journal keyword(s): Galaxy: evolution - Galaxy: formation - Galaxy: halo - stars: abundances - stars: atmospheres - nuclear reactions - nucleosynthesis - abundances

VizieR on-line data: <Available at CDS (J/A+A/668/A168): abund.dat lines.dat>

Simbad objects: 49

goto Full paper

goto View the references in ADS

Number of rows : 49
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 TYC 4-369-1 * 00 08 36.0210546672 +02 58 01.664442732   12.67 11.04     ~ 2 0
2 BD+04 18 * 00 12 49.9034980920 +05 37 39.350587584   11.14 9.69     K5 7 0
3 TYC 33-446-1 * 01 54 22.1680605864 +03 41 45.302784072   11.88 10.47     ~ 2 0
4 TYC 2824-1963-1 * 01 58 38.9289646440 +41 46 30.350491284   11.89 10.69     ~ 2 0
5 TYC 4331-136-1 * 03 57 14.1908017656 +69 44 45.114064728   11.85 10.40     ~ 3 0
6 HD 87740 * 10 07 10.2530783808 +03 41 23.254723068   9.83 8.87     G8III 14 0
7 BD+31 2143 Pe* 10 28 17.2289273064 +30 26 29.237447724   10.20 9.21     G2 7 0
8 HD 91276 * 10 32 57.3735280560 +35 22 56.632261980 10.750 9.920 8.860     G5 11 1
9 BD+13 2383 * 11 17 37.0669603368 +12 24 09.961794072   9.90 8.73     K0 3 0
10 BD-07 3523 * 13 00 33.5954347872 -07 59 38.171837400   10.84 9.66     ~ 2 0
11 HD 115575 * 13 18 09.9656232840 -13 58 45.788514240   10.65 9.59     G2/5(III) 8 0
12 BD+48 2167 Pe* 13 59 19.7422244016 +48 05 35.516919444   10.79 9.75     G0 16 0
13 BD+06 2880 * 14 25 10.3115098200 +06 07 14.931561684   10.85 9.59     K0 4 0
14 BD+32 2483 Em* 14 31 38.9607381288 +31 58 58.392888240   11.28 10.28     G3 5 0
15 BD+41 2520 * 14 42 02.5413183528 +41 14 11.552691660   10.68 9.15 8.4   K5 6 0
16 HD 130971 * 14 51 15.6759217992 -08 59 01.802772132   10.59 9.16     K2III 5 0
17 BD+24 2817 * 15 05 56.8095386088 +24 05 51.677153520   10.03 8.83     K7 3 0
18 HD 238439 Em* 15 17 00.5755671768 +54 35 38.608805292   11.02 9.81     G5 7 0
19 HD 138934 SB* 15 34 21.3751904664 +23 12 36.632085984   9.43 8.37     K2 17 0
20 HD 139423 PM* 15 37 45.8311025616 +11 36 11.604034512   9.68 8.44 7.6   K0 15 0
21 HD 142614 * 15 55 15.3831500928 +08 13 27.843694248   10.31 9.16     K0 7 0
22 HD 143348 * 15 58 36.5466868608 +34 11 33.397511496   9.83 8.73     K2 11 0
23 BD+11 2896 * 16 01 04.8712232952 +11 12 56.241234036   10.34 9.14     K0 4 0
24 BD+20 3298 * 16 36 33.1460951184 +20 25 46.068157308   10.59 9.25     K7 10 0
25 NGC 6205 199 RG* 16 41 32.5304694216 +36 24 42.571380852   12.65 11.93 11.90   ~ 65 0
26 TYC 3085-119-1 RG* 17 16 36.9803928600 +44 10 43.443746256   11.42 10.62     ~ 12 0
27 NAME Sequoia Cluster GlC 17 31 12.0 -39 48 30           ~ 154 0
28 NAME Galactic Center reg 17 45 39.60213 -29 00 22.0000           ~ 16269 0
29 BD+39 3309 * 18 03 47.3520267264 +39 32 31.254227088   10.65 9.83     F5 5 0
30 HD 165400 SB* 18 05 30.4514717568 +09 49 30.377094420   9.69 8.71     K0 5 0
31 TYC 1008-1200-1 * 18 06 31.5844356168 +08 44 54.738107448   12.23 10.74     ~ 2 0
32 2MASS J18564154+2516509 LP? 18 56 41.5459258128 +25 16 50.845111356   12.39 10.81     ~ 2 0
33 TYC 4221-640-1 * 19 09 19.2671708520 +63 03 44.160441984   12.07 11.12     ~ 2 0
34 TYC 4584-784-1 * 19 22 56.4042777072 +76 32 43.280839500   11.87 10.94     ~ 2 0
35 2MASS J20025961+5801071 LP* 20 02 59.6143538448 +58 01 07.126091940   11.91 10.45     ~ 3 0
36 HD 354750 * 20 04 29.0468687904 +13 35 30.995583324   11.76 10.90     G5 5 0
37 BD-00 3963 * 20 17 12.5348456304 +00 21 22.653657216   9.95 8.81     K0 3 0
38 BD+07 4625 PM* 21 07 13.0977435456 +07 44 19.753454364   9.82 8.87     G0 5 0
39 BD+25 4520 * 21 22 08.3242857048 +25 45 15.793984836   11.16 9.78     K0 4 0
40 HD 208316 * 21 55 36.0277286664 -04 13 27.370343136   10.05 8.78     K0V 6 0
41 TYC 4267-2023-1 * 22 01 46.0849927032 +62 27 40.565398716   11.51 10.26     ~ 4 0
42 2MASS J22103877+0516144 LP* 22 10 38.7746372952 +05 16 14.589062940   11.97 10.73     M0.0III 3 0
43 BD+21 4759 * 22 28 46.3550049768 +22 09 11.372774364   10.82 9.79     G0 4 0
44 BD+35 4847 * 22 37 13.4457964272 +36 08 21.560787708   10.31 8.94     K0 4 0
45 GSC 02228-00838 LP? 22 38 23.2790613576 +27 34 24.659669208   11.81 10.32     ~ 2 0
46 BD-00 4538 * 23 38 18.7763376240 +00 46 51.511856880   10.17 9.11     K0 9 0
47 TYC 4001-1161-1 * 23 47 30.714936 +53 47 16.53792   12.93 10.96     ~ 2 0
48 BD+03 4904 SB* 23 55 28.3668835440 +04 21 17.929507068   10.93 9.95     G5 6 0
49 NAME Gaia Enceladus-Sausage St* ~ ~           ~ 860 0

To bookmark this query, right click on this link: simbad:objects in 2022A&A...668A.168C and select 'bookmark this link' or equivalent in the popup menu