HSC 1318

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0.00 UTI
0.51
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.0
Cdup
Radius (P>50% members) 36.9 [arcmin]
  • CN 0.51 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.0 Very likely duplicate

Overview

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HSC 1318 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a very close 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.

Very close Moderate extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Bronze 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 – 64.495 28.206 7.661 8.721 -25.423 15.414
Zhang et al. 2024 64.565 28.25 – – – –
Cavallo et al. 2024 64.903 28.003 7.687 – – –
Hunt & Reffert 2023 64.565 28.25 7.691 8.663 -25.442 23.443

💡 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 – – – – -0.448* – – –
Cavallo et al. 2024 0.14 3.22 – 19 0.320 – – –
Hunt & Reffert 2023 0.13 0.61 1.66 6 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OCSN 268 100.0 64.65 28.2 7.66 8.79 -25.31 14.92 0.39
Taurus 19.2 65.78 27.29 7.72 8.8 -25.91 14.81 0.38

💡 Note: The % column shows the percentage of members that HSC 1318 shares with each listed object.

Visualization

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