HSC 2647

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0.01 UTI
0.0
CN
0.27
Cdens
0.75
CC3
0.0
Clit
0.04
Cdup
Radius (P>50% members) 3.7 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.27 Loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.04 Very likely duplicate

Overview

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HSC 2647 is a sparse, loose object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by very high extinction. It is catalogued as a massive, 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.

Distant Very high extinction Massive Intermediate age

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 216.42 -60.931 0.279 -5.249 -2.918 -69.202
Hunt & Reffert 2024 216.472 -60.934 0.263 -5.244 -2.933 -68.256
Hunt & Reffert 2023 216.472 -60.934 0.263 -5.244 -2.933 -68.256

💡 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] Bfr BSS
Hunt & Reffert 2024 – – – – – 1072* – –
Hunt & Reffert 2023 3.39 5.69 2.13 261 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2797 96.0 216.32 -60.93 0.31 -5.29 -2.94 -69.09 0.54

💡 Note: The % column shows the percentage of members that HSC 2647 shares with each listed object.

Visualization

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