DBSB 61

(MWSC 1919)

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0.10 UTI
0.79
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.18
Cdup
Radius (P>50% members) 1.7 [arcmin]
  • CN 0.79 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.18 Likely duplicate

Overview

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DBSB 61 is a rich, very dense object of very 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

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 168.262 -60.79 0.379 -6.109 1.046 –
Bica et al. 2019 168.256 -60.792 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
NGC 3590 82.4 168.26 -60.79 0.38 -6.11 1.04 – 0.96

💡 Note: The % column shows the percentage of members that DBSB 61 shares with each listed object.

Visualization

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