Dolidze 39

(MWSC 3294)

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0.61 UTI
0.55
CN
1.0
Cdens
0.75
CC3
0.38
Clit
1.0
Cdup
Radius (P>50% members) 2.6 [arcmin]
  • CN 0.55 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.38 Poorly studied
  • Cdup 1.0 Unique

Overview

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Dolidze 39 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate* distance, above the mid-plane, affected by moderate extinction. It is catalogued as an old cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~4.03 kpc) differs significantly from the median photometric distance (~1.92 kpc).

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Relatively close Moderate extinction Old

Dias et al. (2002)
Asterism (Bica, E.; Bonatto, C. 2011, A&A 530, 32)

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 304.07 37.904 0.248 -3.684 -6.026 -1.847
Just et al. 2023 304.045 37.877 – – – –
Loktin & Popova 2017 304.095 37.867 – -0.151 -0.864 –
Kharchenko et al. 2016 304.045 37.877 – – – –
Dias et al. 2014 304.1 37.867 – -0.92 -1.41 –
Kharchenko et al. 2013 304.05 37.88 – -5.97 -2.77 –
Kharchenko et al. 2003 304.11 37.88 – -2.12 -6.08 –

💡 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 – – – 1122 – 155 – –
Loktin & Popova 2017 2.76 0.89 – 1122 – – – –
Kharchenko et al. 2016 1.92 1.81 – 1122 – – – –
Kharchenko et al. 2013 1.92 1.81 – 1122 – – – –
Kharchenko et al. 2003 1.43 1.24 – – – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 1100 85.0 304.07 37.91 0.25 -3.72 -6.01 17.92 0.09

💡 Note: The % column shows the percentage of members that Dolidze 39 shares with each listed object.

Visualization

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