HSC 675

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0.05 UTI
0.0
CN
0.01
Cdens
0.25
CC3
0.0
Clit
0.96
Cdup
Radius (P>50% members) 5.5 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.01 Very loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.96 Unique

Overview

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HSC 675 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This is a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.96) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Very distant Moderate extinction Massive Near-solar metallicity Intermediate age

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 – 315.722 44.768 0.105 -2.602 -3.329 -86.789
Hunt & Reffert 2024 315.711 44.764 0.107 -2.596 -3.344 -86.906
Cavallo et al. 2024 315.743 44.753 0.107 – – –
Hunt & Reffert 2023 315.711 44.764 0.107 -2.596 -3.344 -86.906

💡 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 – – – – – 1221* – –
Cavallo et al. 2024 7.14 1.46 – 813 -0.020 – – –
Hunt & Reffert 2023 8.31 3.62 2.19 104 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FSR 0273 4.0 315.39 44.81 0.18 -2.58 -3.46 -59.07 0.18

💡 Note: The % column shows the percentage of members that HSC 675 shares with each listed object.

Visualization

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