HSC 2985

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0.23 UTI
0.4
CN
0.25
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 6.6 [arcmin]
  • CN 0.4 Poorly populated
  • Cdens 0.25 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 2985 is a poorly populated, loose 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 an extremely metal-poor, very young cluster (see Parameters). It was recently reported in the literature.

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.

Relatively close High extinction Extremely metal-poor Very young

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 266.937 -29.507 0.337 -0.434 -2.079 -15.156
Hunt & Reffert 2024 266.958 -29.536 0.342 -0.431 -2.084 -7.722
Cavallo et al. 2024 266.947 -29.501 0.341 – – –
Hunt & Reffert 2023 266.958 -29.536 0.342 -0.431 -2.084 -7.722

💡 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 – – – – – 742* – –
Cavallo et al. 2024 1.98 4.17 – 13 -2.000 – – –
Hunt & Reffert 2023 2.69 3.24 2.46 11 – – – –

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

Visualization

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