HSC 2827

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0.27 UTI
0.27
CN
0.34
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 11.5 [arcmin]
  • CN 0.27 Poorly populated
  • Cdens 0.34 Loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2827 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Relatively close Low 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 – 250.836 -43.629 0.837 1.483 -2.99 -19.623
Hunt & Reffert 2024 250.763 -43.625 0.852 1.511 -3.005 -17.239
Cavallo et al. 2024 250.79 -43.642 0.84 – – –
Hunt & Reffert 2023 250.763 -43.625 0.852 1.511 -3.005 -17.239

💡 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 – – – – – 96* – –
Cavallo et al. 2024 1.12 0.82 – 427 0.380 – – –
Hunt & Reffert 2023 1.13 1.17 0.67 129 – – – –

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

Visualization

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