HSC 513

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0.09 UTI
0.0
CN
0.07
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 2.8 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.07 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 513 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by high extinction. It is catalogued as a massive, very metal-poor, 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.

Very distant High extinction Massive Very metal-poor Young

Cavallo et al. (2024)
Wood sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 297.459 27.891 0.117 -2.883 -5.291 -38.552
Hunt & Reffert 2024 297.457 27.895 0.095 -2.896 -5.286 -21.638
Cavallo et al. 2024 297.57 27.876 0.096 – – –
Hunt & Reffert 2023 297.457 27.895 0.095 -2.896 -5.286 -21.638

💡 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 – – – – – 1293* – –
Cavallo et al. 2024 5.13 4.36 – 112 -1.040 – – –
Hunt & Reffert 2023 9.05 4.23 2.71 40 – – – –

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

Visualization

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