DB2001 20

(MWSC 3385)

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0.06 UTI
0.0
CN
0.17
Cdens
0.62
CC3
0.0
Clit
0.36
Cdup
Stellar density (N50/rad) 0.9 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.17 Very loose
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.36 Possibly duplicate

Overview

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DB2001 20 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate* distance, above the mid-plane, affected by high extinction. It is catalogued as a low-mass, young cluster (see Parameters). It is rarely studied in the literature.

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

(*): The parallax distance estimate (~3.60 kpc) differs significantly from the median photometric distance (~1.82 kpc).

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.36) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 309.711 42.797 0.278 -3.466 -4.96 –
Just et al. 2023 309.649 42.654 – – – –
Kharchenko et al. 2016 309.649 42.654 – – – –
Kharchenko et al. 2013 309.654 42.657 – 0.78 -0.7 –

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

Reference Year Dist [kpc] Av [mag] DAv [mag] Age [Myr] [Fe/H] [dex] Mass [Msun] Bfrac BSS
UCC 99999– 1.82 3.87 – 32 – 43 – –
Just et al. 2023 – – – 32 – 43 – –
Kharchenko et al. 2016 1.82 3.87 – 32 – – – –
Kharchenko et al. 2013 1.82 3.87 – 32 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
W 75 N 64.0 309.72 42.76 0.23 -3.49 -4.86 – 0.14

💡 Note: The % column shows the percentage of members that DB2001 20 shares with each listed object.

Visualization

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