HSC 787

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0.28 UTI
0.0
CN
1.0
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 1.2 [arcmin]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 787 is a sparse, very dense object of low C3 quality. Its parallax locates it at a moderate* distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~4.60 kpc) differs significantly from the median photometric distance (~3.52 kpc).

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

Distant High 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 – 331.281 56.333 0.217 -3.668 -2.893 -84.034
Hunt & Reffert 2024 331.275 56.333 0.207 -3.66 -2.879 -69.74
Cavallo et al. 2024 331.275 56.334 0.207 – – –
Hunt & Reffert 2023 331.275 56.333 0.207 -3.66 -2.879 -69.74

💡 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 – – – – – 703* – –
Cavallo et al. 2024 2.79 3.33 – 363 0.260 – – –
Hunt & Reffert 2023 4.25 3.74 1.30 38 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3399 76.0 331.27 56.34 0.22 -3.65 -2.9 -84.03 0.06

💡 Note: The % column shows the percentage of members that HSC 787 shares with each listed object.

Visualization

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