HSC 1155

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0.07 UTI
0.0
CN
0.11
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 78.3 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.11 Very loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1155 is a sparse, very loose object of low C3 quality. Its parallax locates it at a very close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age 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 close Low extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Silver sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 37.401 40.629 3.493 -3.729 -12.464 -3.717
Zhang et al. 2024 39.984 40.556 – – – –
Cavallo et al. 2024 38.711 40.437 3.508 – – –
Hunt & Reffert 2023 39.984 40.556 3.488 -3.867 -12.664 -8.058

💡 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
Zhang et al. 2024 – – – – 0.057* – – –
Cavallo et al. 2024 0.30 0.38 – 126 0.050 – – –
Hunt & Reffert 2023 0.28 0.16 0.67 203 – – – –

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

Visualization

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