HSC 2897

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0.01 UTI
0.0
CN
0.52
Cdens
0.62
CC3
0.0
Clit
0.04
Cdup
Stellar density (N50/rad) 2.6 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.52 Moderately dense
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.04 Very likely duplicate

Overview

â„šī¸
HSC 2897 is a sparse, moderately dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by high extinction. It is catalogued as a 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. See table with shared members information.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.04) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Palma et al. (2025)
Part of multiple system G17, along with Bochum_13, NGC_6334 and CWNU_1832.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 259.205 -36.36 0.562 -0.201 -2.225 -403.309
Hunt & Reffert 2024 259.137 -36.376 0.578 -0.129 -2.248 –
Hunt & Reffert 2023 259.137 -36.376 0.578 -0.129 -2.248 –

💡 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– 1.67 3.44 2.38 22 – 261 – –
Hunt & Reffert 2024 – – – – – 261(1) – –
Hunt & Reffert 2023 1.67 3.44 2.38 22 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
DBSB 122 96.0 259.25 -36.35 0.56 -0.16 -2.22 -76.6 0.46
DBSB 123 56.0 259.27 -36.32 0.56 -0.2 -2.21 – 0.34

💡 Note: The % column shows the percentage of members that HSC 2897 shares with each listed object.

Visualization

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