HSC 1480

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0.30 UTI
0.27
CN
0.09
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 0.5 [N/pc2]
  • CN 0.27 Poorly populated
  • Cdens 0.09 Very loose
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1480 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a large* distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~5.83 kpc) differs significantly from the median photometric distance (~4.41 kpc).

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

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 99999– 91.414 23.516 0.171 0.266 -0.416 –
Zhang et al. 2024 91.429 23.511 – – – –
Hunt & Reffert 2024 91.429 23.511 0.185 0.274 -0.429 –
Cavallo et al. 2024 91.411 23.506 0.185 – – –
Hunt & Reffert 2023 91.429 23.511 0.185 0.274 -0.429 –

💡 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] Bfrac BSS
UCC 99999– 4.405 1.725 2.5 154 0.300 688 – –
Hunt & Reffert 2024 – – – – – 688(1) – –
Cavallo et al. 2024 4.13 1.37 – 263 0.300 – – –
Hunt & Reffert 2023 4.68 2.08 2.50 44 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4050 92.6 91.4 23.51 0.17 0.25 -0.42 – 0.03

💡 Note: The % column shows the percentage of members that HSC 1480 shares with each listed object.

Visualization

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