HSC 370

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0.41 UTI
0.56
CN
0.74
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 4.6 [arcmin]
  • CN 0.56 Moderately populated
  • Cdens 0.74 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 370 is a moderately populated, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.

Relatively close High extinction Massive Near-solar metallicity 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 – 288.266 8.546 0.324 -1.64 -3.841 22.1
Hunt & Reffert 2024 288.266 8.543 0.329 -1.607 -3.848 33.203
Cavallo et al. 2024 288.296 8.553 0.324 – – –
Hunt & Reffert 2023 288.266 8.543 0.329 -1.607 -3.848 33.203

💡 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 – – – – – 1013* – –
Cavallo et al. 2024 3.10 4.71 – 27 -0.030 – – –
Hunt & Reffert 2023 2.86 4.54 2.70 66 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4263 74.6 288.26 8.55 0.32 -1.67 -3.84 22.1 0.05

💡 Note: The % column shows the percentage of members that HSC 370 shares with each listed object.

Visualization

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