HSC 1309

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0.05 UTI
0.0
CN
0.05
Cdens
0.75
CC3
0.25
Clit
0.2
Cdup
Stellar density (N50/rad) 0.3 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.05 Very loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 0.2 Likely duplicate

Overview

â„šī¸
HSC 1309 is a sparse, very loose object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a massive, 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.

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

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 99999– 81.287 40.926 0.2 0.168 -0.259 –
Zhang et al. 2024 81.281 40.968 – – – –
Hunt & Reffert 2024 81.281 40.968 0.198 0.179 -0.257 -12.764
Cavallo et al. 2024 81.26 40.986 0.199 – – –
Hunt & Reffert 2023 81.281 40.968 0.198 0.179 -0.257 -12.764

💡 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] Bfrac BSS
UCC 99999– 3.915 1.915 2.19 96 -0.196 1375 – –
Zhang et al. 2024 – – – – 0.009(1) – – –
Hunt & Reffert 2024 – – – – – 1375(1) – –
Cavallo et al. 2024 3.60 2.23 – 37 -0.400 – – –
Hunt & Reffert 2023 4.23 1.60 2.19 156 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 2036 80.0 81.26 40.93 0.21 0.21 -0.25 8.93 0.27

💡 Note: The % column shows the percentage of members that HSC 1309 shares with each listed object.

Visualization

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