HSC 1740

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0.03 UTI
0.26
CN
1.0
Cdens
0.62
CC3
0.0
Clit
0.08
Cdup
Stellar density (N50/rad) 33.5 [N/pc2]
  • CN 0.26 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.08 Very likely duplicate

Overview

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HSC 1740 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, intermediate-age cluster, but with a large variance across recent sources for the age parameter (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.

(*): The parallax distance estimate (~1.32 kpc) differs significantly from the median photometric distance (~2.41 kpc).

Palma et al. (2025)
Classified as genetic pair P187, along with BDSB_93.

Cavallo et al. (2024)
Wood 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– 104.922 -7.793 0.759 -2.415 1.096 4.347
Hunt & Reffert 2024 104.923 -7.801 0.759 -2.419 1.137 25.987
Cavallo et al. 2024 104.888 -7.809 0.762 – – –
Hunt & Reffert 2023 104.923 -7.801 0.759 -2.419 1.137 25.987

💡 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– 2.41 1.565 1.52 158 -0.040 132 – –
Hunt & Reffert 2024 – – – – – 132(1) – –
Cavallo et al. 2024 3.56 1.43 – 309 -0.040 – – –
Hunt & Reffert 2023 1.26 1.70 1.52 8 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
L 1654 92.3 104.92 -7.79 0.73 -2.39 1.1 26.02 0.44

💡 Note: The % column shows the percentage of members that HSC 1740 shares with each listed object.

Visualization

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