LS 139

(La Serena 139)

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0.15 UTI
0.0
CN
0.66
Cdens
0.12
CC3
0.0
Clit
0.96
Cdup
Radius (P>50% members) 3.5 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.66 Moderately dense
  • CC3 0.12 Very low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.96 Unique

Overview

â„šī¸
LS 139 is a sparse, moderately dense object of very low 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.

Note: This is a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.96) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

No fundamental parameters

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 211.523 -61.574 0.385 -7.465 -2.602 -22.874
Bica et al. 2019 211.501 -61.589 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
VVV 035 4.0 211.61 -61.45 0.35 -7.69 -2.83 -51.93 0.14

💡 Note: The % column shows the percentage of members that LS 139 shares with each listed object.

Visualization

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