HSC 1510

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0.02 UTI
0.25
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.04
Cdup
Stellar density (N50/rad) 6.9 [N/pc2]
  • CN 0.25 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.04 Very likely duplicate

Overview

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HSC 1510 is a poorly populated, 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 an intermediate-age 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.

Palma et al. (2025)
Classified as tidal capture (resonant trapping pair) P29, along with HSC_1511.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 91.904 19.156 0.475 -0.13 -1.1 14.478
Hunt & Reffert 2024 91.933 19.169 0.492 -0.13 -1.115 –
Hunt & Reffert 2023 91.933 19.169 0.492 -0.13 -1.115 –

💡 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– 1.99 2.44 0.7 324 – 412 – –
Hunt & Reffert 2024 – – – – – 412(1) – –
Hunt & Reffert 2023 1.99 2.44 0.70 324 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FSR 0903 96.0 91.89 19.13 0.41 -0.15 -1.13 14.48 0.63
FSR 0904 4.0 91.76 19.02 0.46 -0.5 -1.11 35.95 0.86

💡 Note: The % column shows the percentage of members that HSC 1510 shares with each listed object.

Visualization

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