HSC 149

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0.00 UTI
0.0
CN
1.0
Cdens
0.62
CC3
0.0
Clit
0.0
Cdup
Stellar density (N50/rad) 30.7 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.0 Very likely duplicate

Overview

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HSC 149 is a sparse, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a very young 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, and a significant percentage with at least one entry reported in the same catalogue. See table with shared members information.

Palma et al. (2025)
Classified as optical pair (not dynamically associated) P106, along with CWNU_1917.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 273.498 -19.522 0.403 0.144 -2.139 9.859
Hunt & Reffert 2024 273.5 -19.504 0.414 0.137 -2.126 8.569
Hunt & Reffert 2023 273.5 -19.504 0.414 0.137 -2.126 8.569

💡 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– 2.49 3.32 2.13 18 – 281 – –
Hunt & Reffert 2024 – – – – – 281(1) – –
Hunt & Reffert 2023 2.49 3.32 2.13 18 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 288 100.0 273.49 -19.51 0.38 0.15 -2.13 9.86 0.55
HSC 148 56.0 273.5 -19.52 0.35 0.17 -2.17 -11.44 0.0

💡 Note: The % column shows the percentage of members that HSC 149 shares with each listed object.

Visualization

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