HSC 1455

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0.17 UTI
0.0
CN
0.09
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 16.0 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.09 Very loose
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 1455 is a sparse, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

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 Moderate extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 92.291 27.173 0.64 -1.192 -4.731 –
Zhang et al. 2024 92.259 27.199 – – – –
Hunt & Reffert 2024 92.259 27.199 0.653 -1.194 -4.719 –
Cavallo et al. 2024 92.288 27.143 0.652 – – –
Hunt & Reffert 2023 92.259 27.199 0.653 -1.194 -4.719 –

💡 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 – – – – -0.494* – – –
Hunt & Reffert 2024 – – – – – 51* – –
Cavallo et al. 2024 1.59 1.21 – 200 -0.220 – – –
Hunt & Reffert 2023 1.45 0.80 0.59 278 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4136 96.0 92.29 27.17 0.64 -1.19 -4.7 – 0.0

💡 Note: The % column shows the percentage of members that HSC 1455 shares with each listed object.

Visualization

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