UBC 1084

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0.60 UTI
0.76
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.0 [arcmin]
  • CN 0.76 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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UBC 1084 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high 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 large percentage of members with 2 later reported entries. See table with shared members information.

Relatively close High 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 – 300.909 32.685 0.464 -1.074 -2.001 15.65
Hunt & Reffert 2024 300.911 32.675 0.462 -1.055 -2.016 41.494
Cavallo et al. 2024 300.911 32.657 0.466 – – –
Hunt & Reffert 2023 300.911 32.675 0.462 -1.055 -2.016 41.494
Castro-Ginard et al. 2022 300.91 32.68 0.46 -1.06 -2.02 –

💡 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 – – – – – 665* – –
Cavallo et al. 2024 2.24 3.58 – 41 -0.020 – – –
Hunt & Reffert 2023 2.06 3.45 2.53 75 – – – –
Castro-Ginard et al. 2022 2.35 2.75 – 158 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 456 97.4 300.91 32.69 0.46 -1.07 -2.0 51.4 0.04
CWWDL 2459 54.8 300.91 32.68 0.45 -1.06 -2.01 87.15 0.0

💡 Note: The % column shows the percentage of members that UBC 1084 shares with each listed object.

Visualization

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