HSC 135

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0.44 UTI
0.43
CN
1.0
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 6.8 [arcmin]
  • CN 0.43 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 135 is a poorly populated, very 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, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Relatively close Moderate extinction Near-solar metallicity Intermediate age

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 – 271.75 -19.785 0.751 2.778 -0.859 -29.612
Hunt & Reffert 2024 271.739 -19.764 0.743 2.781 -0.826 -21.73
Cavallo et al. 2024 271.775 -19.765 0.743 – – –
Hunt & Reffert 2023 271.739 -19.764 0.743 2.781 -0.826 -21.73

💡 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 – – – – – 217* – –
Cavallo et al. 2024 1.14 1.25 – 457 -0.240 – – –
Hunt & Reffert 2023 1.28 1.35 2.28 91 – – – –

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

Visualization

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