HSC 1134

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0.33 UTI
0.27
CN
1.0
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 6.9 [arcmin]
  • CN 0.27 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1134 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.
Relatively close Moderate extinction Near-solar metallicity Very young

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 – 50.867 59.009 0.977 -0.426 -1.147 -7.984
Hunt & Reffert 2024 50.876 59.001 0.981 -0.428 -1.128 -8.32
Cavallo et al. 2024 50.762 59.011 0.989 – – –
Hunt & Reffert 2023 50.876 59.001 0.981 -0.428 -1.128 -8.32

💡 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 – – – – – 70* – –
Cavallo et al. 2024 1.31 1.96 – 12 -0.030 – – –
Hunt & Reffert 2023 0.98 1.74 1.22 7 – – – –

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

Visualization

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