Dolidze 46

(MWSC 3724)

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0.11 UTI
0.0
CN
0.06
Cdens
0.25
CC3
0.13
Clit
1.0
Cdup
Core radius and density 1.7 [pc], 0.3 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.06 Very loose
  • CC3 0.25 Low quality
  • Clit 0.13 Rarely studied
  • Cdup 1.0 Unique

Overview

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Dolidze 46 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate* distance, below the mid-plane, affected by low extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is rarely studied in the literature.

(*): The parallax distance estimate (~4.03 kpc) differs significantly from the median photometric distance (~1.45 kpc).

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Bica et al. (2019)
Web updates in DAML02, some were later removed (2003 to 2010). Asterisms and cluster alikes by B. Alessi reported in DAML02.

Dias et al. (2002)
Asterism (Archinal, B. A. & Hynes, S. J. 2003); cat V3.5 (Jan 2016)

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 350.499 55.75 0.248 -3.452 -1.419 –
Just et al. 2023 350.507 55.742 – – – –
Dib et al. 2018 350.514 55.745 – – – –
Joshi et al. 2016 350.514 55.745 – – – –
Kharchenko et al. 2016 350.507 55.742 – – – –
Kharchenko et al. 2013 350.514 55.745 – -2.38 -1.97 –
Kharchenko et al. 2012 350.514 55.745 – -2.38 -1.97 –

💡 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– 1.45 0.95 – 258 – 54 – –
Just et al. 2023 – – – 258 – 54 – –
Dib et al. 2018 1.45 – – 258 – – – –
Joshi et al. 2016 1.45 0.95 – 258 – – – –
Kharchenko et al. 2016 1.45 0.95 – 258 – – – –
Kharchenko et al. 2013 1.45 0.95 – 258 – – – –
Kharchenko et al. 2012 1.45 0.95 – 258 – – – –

Visualization

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