HSC 1685

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0.05 UTI
0.0
CN
0.04
Cdens
0.25
CC3
0.0
Clit
0.96
Cdup
Radius (P>50% members) 6.5 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.04 Very loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.96 Unique

Overview

â„šī¸
HSC 1685 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large* distance, near 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.

(*): The parallax distance estimate (~5.46 kpc) differs significantly from the median photometric distance (~4.07 kpc).

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.

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 – 103.308 -0.638 0.183 -0.195 0.603 59.723
Hunt & Reffert 2024 103.306 -0.657 0.199 -0.238 0.624 –
Cavallo et al. 2024 103.355 -0.588 0.198 – – –
Hunt & Reffert 2023 103.306 -0.657 0.199 -0.238 0.624 –

💡 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 – – – – – 158* – –
Cavallo et al. 2024 3.77 1.79 – 76 0.120 – – –
Hunt & Reffert 2023 4.37 1.85 1.57 48 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 2058 4.0 103.43 -0.49 0.2 -0.38 0.49 78.49 0.03

💡 Note: The % column shows the percentage of members that HSC 1685 shares with each listed object.

Visualization

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