HSC 807

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0.41 UTI
0.28
CN
1.0
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 1.3 [arcmin]
  • CN 0.28 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 807 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young 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.

Distant Moderate extinction Near-solar metallicity Young

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 – 336.733 55.638 0.216 -3.589 -3.079 –
Hunt & Reffert 2024 336.731 55.64 0.23 -3.596 -3.079 –
Cavallo et al. 2024 336.714 55.644 0.228 – – –
Hunt & Reffert 2023 336.731 55.64 0.23 -3.596 -3.079 –

💡 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 – – – – – 423* – –
Cavallo et al. 2024 4.31 1.71 – 41 0.490 – – –
Hunt & Reffert 2023 4.16 1.70 0.59 17 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3224 96.4 336.73 55.66 0.22 -3.59 -3.06 -73.55 0.18

💡 Note: The % column shows the percentage of members that HSC 807 shares with each listed object.

Visualization

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