Dolidze 17

(MWSC 513)

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0.06 UTI
0.0
CN
0.0
Cdens
0.12
CC3
0.1
Clit
1.0
Cdup
Core radius and density 3.8 [pc], 0.02 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.0 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.1 Rarely studied
  • Cdup 1.0 Unique

Overview

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Dolidze 17 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a large* distance, well below the mid-plane, affected by moderate extinction. It is catalogued as a low-mass, old cluster (see Parameters). It is rarely studied in the literature.

(*): The parallax distance estimate (~8.13 kpc) differs significantly from the median photometric distance (~1.03 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)
Analysis of Dolidze objects by M. Kronberger reported in DAML02. Web updates in DAML02, some were later removed (2003 to 2010).

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– 80.605 7.157 0.123 0.083 -0.641 122.596
Just et al. 2023 80.625 7.161 – – – –
Dib et al. 2018 80.632 7.16 – – – –
Joshi et al. 2016 80.632 7.16 – – – –
Kharchenko et al. 2016 80.625 7.161 – – – –
Kharchenko et al. 2013 80.632 7.16 – -0.5 -6.51 –

💡 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– 1.03 1.31 – 1514 – 20 – –
Just et al. 2023 – – – 1514 – 20 – –
Dib et al. 2018 1.03 – – 1514 – – – –
Joshi et al. 2016 1.03 1.31 – 1514 – – – –
Kharchenko et al. 2016 1.03 1.31 – 1514 – – – –
Kharchenko et al. 2013 1.03 1.31 – 1514 – – – –

Visualization

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