HSC 1848

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0.03 UTI
0.3
CN
0.14
Cdens
0.12
CC3
0.0
Clit
0.3
Cdup
Radius (P>50% members) 7.3 [arcmin]
  • CN 0.3 Poorly populated
  • Cdens 0.14 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.3 Possibly duplicate

Overview

â„šī¸
HSC 1848 is a poorly populated, very loose object of very low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

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

Relatively close Low extinction Near-solar metallicity Intermediate age

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 – 109.576 -20.051 0.325 -2.086 3.284 –
Hunt & Reffert 2024 109.575 -20.058 0.314 -2.077 3.283 66.25
Cavallo et al. 2024 109.749 -19.806 0.314 – – –
Hunt & Reffert 2023 109.575 -20.058 0.314 -2.077 3.283 66.25

💡 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 – – – – – 73* – –
Cavallo et al. 2024 2.31 0.93 – 245 -0.320 – – –
Hunt & Reffert 2023 2.75 0.91 2.22 257 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 3813 70.0 109.57 -20.05 0.32 -2.02 3.31 – 0.16

💡 Note: The % column shows the percentage of members that HSC 1848 shares with each listed object.

Visualization

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