OC 0650

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0.42 UTI
0.0
CN
0.59
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 1.6 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.59 Moderately dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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OC 0650 is a sparse, moderately dense object of very high C3 quality. Its parallax locates it at a large* distance, below the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~5.98 kpc) differs significantly from the median photometric distance (~4.28 kpc).

Note: This object shares a significant percentage of members with at least one entry reported in the same catalogue. See table with shared members information.

Distant High extinction Massive Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 244.584 -51.529 0.167 -2.742 -2.784 -26.929
Hunt & Reffert 2024 244.586 -51.531 0.169 -2.765 -2.812 -26.967
Cavallo et al. 2024 244.589 -51.527 0.167 – – –
Hunt & Reffert 2023 244.586 -51.531 0.169 -2.765 -2.812 -26.967
Hao et al. 2022 244.585 -51.54 0.157 -2.746 -2.784 –

💡 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
Hunt & Reffert 2024 – – – – – 2404* – –
Cavallo et al. 2024 3.22 4.75 – 263 -0.260 – – –
Hunt & Reffert 2023 5.33 4.59 2.61 161 – – – –
Hao et al. 2022 – 0.34 – 794 0.274 – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0651 72.0 244.6 -51.52 0.15 -2.74 -2.79 -26.93 0.4

💡 Note: The % column shows the percentage of members that OC 0650 shares with each listed object.

Visualization

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