HSC 245

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0.08 UTI
0.0
CN
1.0
Cdens
0.38
CC3
0.0
Clit
0.28
Cdup
Stellar density (N50/rad) 5.7 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.28 Possibly duplicate

Overview

â„šī¸
HSC 245 is a sparse, very dense object of low C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by very high extinction. It is catalogued as a very young 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.

(*): The parallax distance estimate (~2.86 kpc) differs significantly from the median photometric distance (~2.15 kpc).

Palma et al. (2025)
Part of multiple system G156, along with UBC_1033, HSC_250 and HSC_249.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 279.897 -7.054 0.35 0.006 -1.955 26.091
Hunt & Reffert 2024 279.885 -7.06 0.437 -0.001 -1.923 -6.42
Hunt & Reffert 2023 279.885 -7.06 0.437 -0.001 -1.923 -6.42

💡 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– 2.15 5.15 1.55 7 – 398 – –
Hunt & Reffert 2024 – – – – – 398(1) – –
Hunt & Reffert 2023 2.15 5.15 1.55 7 – – – –

(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 2543 72.0 279.9 -7.04 0.29 0.02 -1.98 28.71 0.65

💡 Note: The % column shows the percentage of members that HSC 245 shares with each listed object.

Visualization

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