LS 125

(La Serena 125)

Click to load Aladin Lite
0.05 UTI
0.76
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.1
Cdup
Radius (P>50% members) 1.2 [arcmin]
  • CN 0.76 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.1 Likely duplicate

Overview

â„šī¸
LS 125 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane. No fundamental parameter values are available for this object. It is rarely studied in the literature, with no articles listed in the last 7 years.

âš ī¸ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

No fundamental parameters

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 209.661 -61.676 0.263 -6.126 -2.413 -41.574
Bica et al. 2019 209.648 -61.67 – – – –

💡 Note: The UCC values are estimated from its identified members.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
SAI 120 90.0 209.67 -61.68 0.26 -6.11 -2.4 -40.83 0.5
CWNU 3943 75.0 209.66 -61.68 0.23 -6.1 -2.4 -41.57 0.02

💡 Note: The % column shows the percentage of members that LS 125 shares with each listed object.

Visualization

â„šī¸