HSC 361

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0.39 UTI
0.36
CN
0.84
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 7.6 [arcmin]
  • CN 0.36 Poorly populated
  • Cdens 0.84 Dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 361 is a poorly populated, dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
Relatively close Moderate extinction Near-solar metallicity 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 – 288.404 6.357 0.756 -2.11 -4.249 -25.606
Hunt & Reffert 2024 288.397 6.404 0.745 -2.099 -4.24 -25.6
Cavallo et al. 2024 288.417 6.384 0.743 – – –
Hunt & Reffert 2023 288.397 6.404 0.745 -2.099 -4.24 -25.6

💡 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 – – – – – 205* – –
Cavallo et al. 2024 1.43 1.44 – 49 0.340 – – –
Hunt & Reffert 2023 1.26 1.44 1.26 76 – – – –

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

Visualization

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