HSC 2848

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0.08 UTI
0.0
CN
0.3
Cdens
0.75
CC3
0.0
Clit
0.36
Cdup
Stellar density (N50/rad) 1.5 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.3 Loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.36 Possibly duplicate

Overview

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HSC 2848 is a sparse, loose object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate 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, and a very small 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 P151, along with OC_0673.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 253.535 -41.155 0.614 -0.573 -1.71 -15.696
Hunt & Reffert 2024 253.494 -41.156 0.62 -0.583 -1.702 –
Hunt & Reffert 2023 253.494 -41.156 0.62 -0.583 -1.702 –

💡 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– 1.55 1.33 0.37 11 – 119 – –
Hunt & Reffert 2024 – – – – – 119(1) – –
Hunt & Reffert 2023 1.55 1.33 0.37 11 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 553 64.0 253.51 -41.26 0.6 -0.54 -1.8 -17.48 0.44
HSC 2849 8.0 253.65 -40.99 0.6 -0.46 -1.59 -33.1 0.42

💡 Note: The % column shows the percentage of members that HSC 2848 shares with each listed object.

Visualization

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