HSC 1845

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0.35 UTI
0.27
CN
0.97
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 2.3 [arcmin]
  • CN 0.27 Poorly populated
  • Cdens 0.97 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1845 is a poorly populated, very dense object of intermediate 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.
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 – 111.672 -18.759 0.283 -1.599 2.198 –
Hunt & Reffert 2024 111.679 -18.755 0.29 -1.59 2.181 –
Cavallo et al. 2024 111.671 -18.769 0.288 – – –
Hunt & Reffert 2023 111.679 -18.755 0.29 -1.59 2.181 –

💡 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 – – – – – 342* – –
Cavallo et al. 2024 3.56 2.04 – 37 0.200 – – –
Hunt & Reffert 2023 3.19 1.75 1.20 93 – – – –

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

Visualization

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