HSC 1917

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0.23 UTI
0.0
CN
0.38
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 2.0 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.38 Loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 1917 is a sparse, loose object of high C3 quality. Its parallax locates it at a large* distance, near the mid-plane, affected by moderate extinction. It is catalogued as a metal-poor, young cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~5.84 kpc) differs significantly from the median photometric distance (~4.40 kpc).

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.

Distant Moderate extinction Metal-poor 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 – 116.335 -24.004 0.171 -1.257 1.974 –
Hunt & Reffert 2024 116.347 -24.004 0.176 -1.27 1.948 –
Cavallo et al. 2024 116.334 -24.021 0.176 – – –
Hunt & Reffert 2023 116.347 -24.004 0.176 -1.27 1.948 –

💡 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 – – – – – 283* – –
Cavallo et al. 2024 3.84 1.59 – 20 -0.560 – – –
Hunt & Reffert 2023 4.96 1.31 0.78 72 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3272 100.0 116.33 -24.0 0.19 -1.26 1.98 59.71 0.13

💡 Note: The % column shows the percentage of members that HSC 1917 shares with each listed object.

Visualization

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