HSC 145

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0.36 UTI
0.28
CN
1.0
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 4.8 [arcmin]
  • CN 0.28 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 145 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near 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.

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

Relatively close Moderate extinction Near-solar metallicity Very 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 – 271.374 -18.778 0.9 2.631 2.072 -22.212
Hunt & Reffert 2024 271.388 -18.771 0.907 2.634 2.119 -21.796
Cavallo et al. 2024 271.388 -18.79 0.906 – – –
Hunt & Reffert 2023 271.388 -18.771 0.907 2.634 2.119 -21.796

💡 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 – – – – – 159* – –
Cavallo et al. 2024 1.17 2.71 – 14 -0.220 – – –
Hunt & Reffert 2023 1.06 1.97 1.65 15 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3380 89.3 271.38 -18.78 0.9 2.64 2.07 -22.6 0.01

💡 Note: The % column shows the percentage of members that HSC 145 shares with each listed object.

Visualization

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