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Query : 1997A&A...322L..29G |
1997A&A...322L..29G - Astronomy and Astrophysics, volume 322, L29-32 (1997/6-3)
What can we learn from the r-element distribution of CS 22892-052?
GORIELY S. and ARNOULD M.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): nucleosynthesis - nuclear reactions - stars: abundances - solar system: general - stars: CS 22892-052 (BPS CS 22892-0052)
Simbad objects: 4
Number of rows : 4 |
N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2022 |
#notes |
---|---|---|---|---|---|---|---|---|---|---|---|---|
1 | SKB 2 | Pe* | 00 41 39.8197621944 | -26 18 54.460585116 | 13.338 | 12.221 | 11.704 | 11.321 | CEMP-s | 88 | 0 | |
2 | HD 140283 | Pe* | 15 43 03.0971190219 | -10 56 00.595693188 | 7.508 | 7.711 | 7.212 | 6.63 | 8.21 | F9VkA5mA1 | 890 | 0 |
3 | HE 2134-3940 | Pe* | 21 37 45.7673945880 | -39 27 22.313379600 | 13.790 | 12.660 | 12.160 | 11.760 | KIIvw | 84 | 0 | |
4 | BPS CS 22892-0052 | Pe* | 22 17 01.6558764360 | -16 39 27.051026544 | 14.03 | 13.20 | 13.06 | 12.19 | KIIvw | 427 | 0 |
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