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Query : 2015A&A...583A..49H |
2015A&A...583A..49H - Astronomy and Astrophysics, volume 583A, 49-49 (2015/11-1)
The role of binaries in the enrichment of the early Galactic halo. I. r-process-enhanced metal-poor stars.
HANSEN T.T., ANDERSEN J., NORDSTROEM B., BEERS T.C., YOON J. and BUCHHAVE L.A.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): stars: abundances - stars: chemically peculiar - binaries: spectroscopic - Galaxy: halo - ISM: structure
Simbad objects: 31
Number of rows : 31 |
N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2024 |
#notes |
---|---|---|---|---|---|---|---|---|---|---|---|---|
1 | HD 20 | Pe* | 00 05 15.3242691048 | -27 16 18.140091852 | 9.65 | 9.40 | 8.865 | 8.377 | F2V | 70 | 0 | |
2 | BPS CS 29497-0004 | Pe* | 00 28 06.9155612016 | -26 03 04.269055032 | 14.76 | 14.07 | 13.583 | 13.116 | ~ | 57 | 0 | |
3 | HD 3765 | PM* | 00 40 49.2698857963 | +40 11 13.823048636 | 8.30 | 6.8 | K2V | 265 | 0 | |||
4 | BPS CS 22183-0031 | Pe* | 01 09 05.0900915136 | -04 43 21.343580436 | 14.24 | 13.62 | 13.178 | 12.724 | ~ | 46 | 0 | |
5 | BD-16 251 | RG* | 01 29 31.1311443552 | -16 00 45.495314460 | 12.527 | 12.427 | 11.642 | 11.189 | 10.713 | CEMP | 291 | 0 |
6 | NAME Magellanic Clouds | GrG | 03 00 | -71.0 | ~ | 7062 | 0 | |||||
7 | HE 0432-0923 | Pe* | 04 34 25.6711921824 | -09 16 50.513595636 | 15.165 | 14.140 | ~ | 14 | 0 | |||
8 | HE 0442-1234 | Pe* | 04 44 51.7052109360 | -12 28 45.533823744 | 12.914 | 11.672 | ~ | 14 | 0 | |||
9 | HE 0524-2055 | Pe* | 05 27 04.4443239912 | -20 52 42.096542448 | 14.013 | 12.937 | ~ | 12 | 0 | |||
10 | HD 38230 | PM* | 05 46 01.8857259248 | +37 17 04.738728231 | 8.19 | 6.8 | K0V | 158 | 0 | |||
11 | HD 79210 | SB* | 09 14 22.7748624830 | +52 41 11.791503353 | 9.388 | 6.8 | K7V | 309 | 0 | |||
12 | HE 1044-2509 | Pe* | 10 47 16.4778519192 | -25 25 18.271615980 | 15.011 | 14.345 | 13.877 | 13.399 | ~ | 9 | 0 | |
13 | HE 1105+0027 | Pe* | 11 07 49.5058798584 | +00 11 38.346763524 | 16.038 | 15.646 | 15.358 | 15.018 | CEMP-s | 27 | 0 | |
14 | HE 1127-1143 | Pe* | 11 29 50.6275439136 | -12 00 12.581828208 | 15.885 | 15.434 | 15.002 | ~ | 14 | 0 | ||
15 | HE 1219-0312 | Pe* | 12 21 34.1430245160 | -03 28 39.636260184 | 15.940 | 15.043 | ~ | 40 | 0 | |||
16 | HD 115444 | Pe* | 13 16 42.4590842616 | +36 22 52.692135420 | 9.77 | 8.97 | 8.3 | 7.88 | G9V | 243 | 0 | |
17 | HD 115404 | PM* | 13 16 51.0514297623 | +17 01 01.840901307 | 7.69 | 6.66 | K2V | 280 | 0 | |||
18 | HD 122563 | Pe* | 14 02 31.8455084952 | +09 41 09.944391876 | 7.47 | 7.10 | 6.19 | 5.37 | 4.79 | G8:III:Fe-5 | 854 | 0 |
19 | HD 122653 | * | 14 02 50.3185495488 | +17 59 16.227716604 | 7.448 | 9.55 | 8.06 | 5.616 | K0 | 17 | 0 | |
20 | HE 1430+0053 | Pe* | 14 33 16.5345630936 | +00 40 48.883742256 | 14.280 | 13.663 | 13.252 | 12.813 | ~ | 16 | 0 | |
21 | HE 1523-0901 | Pe* | 15 26 01.0697532504 | -09 11 38.885639784 | 12.37 | 11.50 | 10.476 | 9.863 | CEMP | 79 | 0 | |
22 | HD 151541 | PM* | 16 42 38.5765856163 | +68 06 07.791412449 | 8.32 | 7.1 | K1 | 133 | 0 | |||
23 | HD 182488 | PM* | 19 23 34.0131683760 | +33 13 19.078425912 | 5.8 | K0V | 279 | 1 | ||||
24 | HD 197076 | PM* | 20 40 45.1407228005 | +19 56 07.930118119 | 7.14 | 7.06 | 6.44 | 5.95 | 5.61 | G5V | 258 | 0 |
25 | BPS CS 22892-0052 | Pe* | 22 17 01.6558764360 | -16 39 27.051026544 | 14.03 | 13.20 | 13.06 | 12.19 | KIIvw | 448 | 0 | |
26 | HE 2224+0143 | Pe* | 22 27 23.1215289240 | +01 58 33.066485508 | 14.54 | 13.83 | 13.208 | 12.733 | ~ | 21 | 0 | |
27 | HE 2244-1503 | Pe* | 22 47 25.8324935880 | -14 47 30.211752372 | 15.351 | 14.483 | ~ | 9 | 0 | |||
28 | HD 221170 | Pe* | 23 29 28.8087143040 | +30 25 57.849303180 | 9.43 | 8.74 | 7.66 | CEMP-r | 289 | 0 | ||
29 | HE 2327-5642 | Pe* | 23 30 37.0896973176 | -56 26 14.385030648 | 14.590 | 13.881 | 13.425 | 12.948 | ~ | 39 | 0 | |
30 | BPS CS 30315-0029 | Pe* | 23 34 26.6960486448 | -26 42 14.003379828 | 14.56 | 13.64 | 13.092 | 12.518 | ~ | 23 | 0 | |
31 | LP 584-32 | Pe* | 23 57 18.9066974952 | -00 52 47.436045024 | 16.366 | 15.636 | 15.141 | 14.673 | F5 | 31 | 0 |
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