DBSB 73

(MWSC 1981)

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0.30 UTI
0.0
CN
1.0
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 2.6 [arcmin]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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DBSB 73 is a sparse, very dense object of intermediate C3 quality. Its parallax locates it at a moderate* distance, below the mid-plane, affected by high extinction. It is catalogued as a very young cluster (see Parameters). It is rarely studied in the literature.

(*): The parallax distance estimate (~2.64 kpc) differs significantly from the median photometric distance (~4.53 kpc).

Distant High extinction Very young

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 177.545 -64.868 0.378 -6.459 0.284 -25.066
Just et al. 2023 177.532 -64.867 – – – –
Kharchenko et al. 2016 177.532 -64.867 – – – –
Kharchenko et al. 2013 177.54 -64.87 – -9.67 -0.06 –

💡 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] Bfr BSS
Just et al. 2023 – – – 3 – 269 – –
Kharchenko et al. 2016 4.53 3.55 – 3 – – – –
Kharchenko et al. 2013 4.53 3.55 – 3 – – – –

Visualization

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