UBC 207

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0.53 UTI
0.48
CN
1.0
Cdens
0.75
CC3
0.25
Clit
0.98
Cdup
Radius (P>50% members) 21.3 [arcmin]
  • CN 0.48 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 0.98 Unique

Overview

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UBC 207 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a very close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is poorly studied in the literature.

Note: This is a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.

Very close Low extinction Near-solar metallicity Very young

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 83.87 -4.615 2.567 1.106 0.57 20.544
Alfonso et al. 2024 83.808 -4.628 2.531 1.126 0.478 –
Celli et al. 2024 83.848 -4.486 – – – –
Cantat-Gaudin et al. 2020 83.848 -4.486 2.544 1.086 0.555 –
Castro-Ginard et al. 2020 83.866 -4.505 2.539 1.071 0.614 –

💡 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
Alfonso et al. 2024 0.37 0.88 – 12 0.001 – – –
Celli et al. 2024 – – – 15 – 123 – –
Cantat-Gaudin et al. 2020 0.38 0.88 – 15 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
OCSN 225 87.5 83.84 -4.96 2.55 1.25 -0.08 22.73 0.36
NGC 1976 2.1 83.82 -5.45 2.58 1.25 0.19 19.86 0.77
OCSN 244 2.1 83.82 -5.43 2.52 1.39 0.33 25.62 0.25

💡 Note: The % column shows the percentage of members that UBC 207 shares with each listed object.

Visualization

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