2019NatAs...3..631X


Query : 2019NatAs...3..631X

2019NatAs...3..631X - Nature Astronomy, 3, 631-635 (2019)

Evidence for the accretion origin of halo stars with an extreme r-process enhancement.

XING Q.-F., ZHAO G., AOKI W., HONDA S., LI H.-N., ISHIGAKI M.N. and MATSUNO T.

Journal keyword(s):

Simbad objects: 11

goto View the references in ADS

Number of rows : 11
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 NAME Sculptor Dwarf Galaxy G 01 00 09.4 -33 42 32   9.79 8.6 8.81   ~ 1498 4
2 MCG-06-07-001 G 02 39 59.3 -34 26 57   9.02 7.4     ~ 1894 1
3 NAME Reticulum II G 03 35 42.1 -54 02 57           ~ 375 0
4 ESO 206-20A G 06 41 36.7 -50 57 58   22.14 11.0 19.47   ~ 1190 0
5 NAME Sextans dSph LSB 10 13 02.9 -01 36 53   12 10.4     ~ 921 0
6 LAMOST J112456.61+453531.3 * 11 24 56.6106775656 +45 35 31.306337916           ~ 13 0
7 Z 318-18 G 15 09 08.0 +67 13 21   13.60 10.6     ~ 1459 0
8 2MASS J15095862+6716200 RB? 15 09 58.6103318448 +67 16 20.032584024   18.53 17.006   15.614 ~ 41 0
9 Z 300-12 G 17 20 14.335 +57 55 16.39   12.40 10.6     ~ 1428 1
10 UCAC2 13007354 Pe* 18 02 42.2736456576 -44 04 42.648519648   13.851 12.621 12.30 11.26 CEMP 19 0
11 HD 222925 Pe* 23 45 17.6074777008 -61 54 42.835286016   9.56 9.03     ApSrEu 83 0

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