HSC 2962

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0.08 UTI
0.0
CN
0.04
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 4.3 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.04 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2962 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large* distance, above 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.

(*): The parallax distance estimate (~7.08 kpc) differs significantly from the median photometric distance (~5.18 kpc).

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Very 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 – 261.854 -29.913 0.141 -1.148 -6.687 -66.942
Hunt & Reffert 2024 261.861 -29.946 0.145 -1.176 -6.667 –
Hunt & Reffert 2023 261.861 -29.946 0.145 -1.176 -6.667 –

💡 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 – – – – – 2332* – –
Hunt & Reffert 2023 5.18 5.98 1.04 308 – – – –

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

Visualization

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