HSC 1981

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0.00 UTI
0.75
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.0
Cdup
Radius (P>50% members) 1.9 [arcmin]
  • CN 0.75 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.0 Very likely duplicate

Overview

â„šī¸
HSC 1981 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Distant 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 – 118.952 -29.473 0.262 -2.629 2.935 78.743
Hunt & Reffert 2024 118.954 -29.474 0.257 -2.62 2.942 70.42
Cavallo et al. 2024 118.948 -29.474 0.261 – – –
Hunt & Reffert 2023 118.954 -29.474 0.257 -2.62 2.942 70.42

💡 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 – – – – – 920* – –
Cavallo et al. 2024 3.24 2.14 – 20 0.050 – – –
Hunt & Reffert 2023 3.36 1.92 1.95 169 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 201 100.0 118.96 -29.47 0.25 -2.62 2.93 70.43 0.61

💡 Note: The % column shows the percentage of members that HSC 1981 shares with each listed object.

Visualization

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