HSC 1351

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0.00 UTI
0.0
CN
0.54
Cdens
0.62
CC3
0.25
Clit
0.0
Cdup
Radius (P>50% members) 4.6 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.54 Moderately dense
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 0.0 Very likely duplicate

Overview

â„šī¸
HSC 1351 is a sparse, moderately dense object of intermediate 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, 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 very likely a duplicate object, which shares a large 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)
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 – 82.1 35.043 0.467 0.101 -1.764 -1.588
Zhang et al. 2024 82.118 35.056 – – – –
Hunt & Reffert 2024 82.118 35.056 0.461 0.116 -1.736 –
Cavallo et al. 2024 82.042 35.045 0.461 – – –
Hunt & Reffert 2023 82.118 35.056 0.461 0.116 -1.736 –

💡 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 – – – – -0.440* – – –
Hunt & Reffert 2024 – – – – – 149* – –
Cavallo et al. 2024 2.22 1.64 – 13 0.500 – – –
Hunt & Reffert 2023 2.05 1.87 1.00 6 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
SAI 50 100.0 82.16 35.03 0.46 0.15 -1.75 0.4 0.45

💡 Note: The % column shows the percentage of members that HSC 1351 shares with each listed object.

Visualization

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