HSC 1723

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0.08 UTI
0.0
CN
0.61
Cdens
0.25
CC3
0.0
Clit
0.48
Cdup
Radius (P>50% members) 3.9 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.61 Moderately dense
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.48 Possibly duplicate

Overview

â„šī¸
HSC 1723 is a sparse, moderately dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 104.85 -4.74 0.433 -1.49 0.693 62.256
Hunt & Reffert 2024 104.838 -4.703 0.445 -1.507 0.705 62.279
Cavallo et al. 2024 104.84 -4.728 0.445 – – –
Hunt & Reffert 2023 104.838 -4.703 0.445 -1.507 0.705 62.279

💡 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 – – – – – 162* – –
Cavallo et al. 2024 2.23 1.27 – 10 0.080 – – –
Hunt & Reffert 2023 2.11 1.18 1.45 10 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Sh2 287C 52.0 104.85 -4.7 0.45 -1.61 0.76 48.19 0.16
BDSB 90 28.0 104.89 -4.81 0.44 -1.49 0.61 62.26 0.28

💡 Note: The % column shows the percentage of members that HSC 1723 shares with each listed object.

Visualization

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