HSC 1341

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0.05 UTI
0.0
CN
0.15
Cdens
0.25
CC3
0.0
Clit
0.6
Cdup
Radius (P>50% members) 17.4 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.15 Very loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.6 Likely unique

Overview

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HSC 1341 is a sparse, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Close Low extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 80.524 35.48 0.94 -0.117 -3.105 -9.214
Zhang et al. 2024 80.256 35.326 – – – –
Cavallo et al. 2024 80.587 35.554 0.965 – – –
Hunt & Reffert 2023 80.256 35.326 0.965 -0.13 -3.158 -5.348

💡 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
Zhang et al. 2024 – – – – -0.213* – – –
Cavallo et al. 2024 1.00 0.55 – 100 0.570 – – –
Hunt & Reffert 2023 0.99 0.92 1.07 49 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1089 40.0 80.07 35.63 0.92 -0.24 -3.11 -14.17 0.15

💡 Note: The % column shows the percentage of members that HSC 1341 shares with each listed object.

Visualization

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