HSC 2540

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0.30 UTI
0.4
CN
0.37
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 7.7 [arcmin]
  • CN 0.4 Poorly populated
  • Cdens 0.37 Loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2540 is a poorly populated, 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 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 – 193.815 -59.022 0.484 -4.665 -0.868 -12.904
Hunt & Reffert 2024 193.753 -59.03 0.486 -4.652 -0.867 -13.005
Cavallo et al. 2024 193.958 -59.022 0.486 – – –
Hunt & Reffert 2023 193.753 -59.03 0.486 -4.652 -0.867 -13.005

💡 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 – – – – – 230* – –
Cavallo et al. 2024 2.00 1.20 – 60 0.060 – – –
Hunt & Reffert 2023 1.98 1.02 0.71 63 – – – –

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

Visualization

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