HSC 1084

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0.25 UTI
0.34
CN
0.3
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 2.6 [arcmin]
  • CN 0.34 Poorly populated
  • Cdens 0.3 Loose
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1084 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a large distance, well above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

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

Very distant 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 – 40.457 67.193 0.159 -0.873 0.339 -57.903
Hunt & Reffert 2024 40.449 67.18 0.157 -0.849 0.336 -57.617
Cavallo et al. 2024 40.437 67.261 0.165 – – –
Hunt & Reffert 2023 40.449 67.18 0.157 -0.849 0.336 -57.617

💡 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 – – – – – 643* – –
Cavallo et al. 2024 5.22 3.20 – 62 0.000 – – –
Hunt & Reffert 2023 5.99 3.23 1.04 113 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3065 97.1 40.45 67.25 0.16 -0.88 0.34 -57.9 0.12

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

Visualization

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