UBC 1229

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0.36 UTI
0.26
CN
0.31
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.8 [arcmin]
  • CN 0.26 Poorly populated
  • Cdens 0.31 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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UBC 1229 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.

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

Relatively close Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 27.678 59.114 0.341 -0.747 -0.416 –
Hunt & Reffert 2024 27.682 59.111 0.33 -0.704 -0.419 –
Cavallo et al. 2024 28.139 59.114 0.331 – – –
Hunt & Reffert 2023 27.682 59.111 0.33 -0.704 -0.419 –
Castro-Ginard et al. 2022 27.68 59.11 0.35 -0.78 -0.42 –

💡 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 – – – – – 168* – –
Cavallo et al. 2024 2.83 1.53 – 95 0.400 – – –
Hunt & Reffert 2023 2.74 1.59 0.60 63 – – – –
Castro-Ginard et al. 2022 3.04 1.40 – 22 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 4603 65.4 27.9 59.1 0.34 -0.71 -0.45 – 0.08

💡 Note: The % column shows the percentage of members that UBC 1229 shares with each listed object.

Visualization

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