Dolidze 29

(MWSC 2937)

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0.08 UTI
0.0
CN
0.01
Cdens
0.12
CC3
0.13
Clit
1.0
Cdup
Core radius and density 8.1 [pc], 0.07 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.01 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.13 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Dolidze 29 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate* distance, above the mid-plane, affected by very high extinction. It is catalogued as a young cluster (see Parameters). It is rarely studied in the literature.

(*): The parallax distance estimate (~3.79 kpc) differs significantly from the median photometric distance (~1.46 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– 277.884 -6.596 0.264 -3.049 -4.425 –
Just et al. 2023 277.842 -6.634 – – – –
Dib et al. 2018 277.849 -6.633 – – – –
Joshi et al. 2016 277.849 -6.633 – – – –
Kharchenko et al. 2016 277.842 -6.634 – – – –
Kharchenko et al. 2013 277.849 -6.633 – -0.73 -1.15 –
Lynga 1987 277.848 -6.627 – – – –

💡 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– 1.46 9.59 – 32 – 339 – –
Just et al. 2023 – – – 32 – 339 – –
Dib et al. 2018 1.46 – – 32 – – – –
Joshi et al. 2016 1.46 9.59 – 32 – – – –
Kharchenko et al. 2016 1.46 9.59 – 32 – – – –
Kharchenko et al. 2013 1.46 9.59 – 32 – – – –

Visualization

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