HSC 2877

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0.40 UTI
0.27
CN
1.0
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 8.0 [arcmin]
  • CN 0.27 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 2877 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.
Close Moderate extinction Near-solar metallicity Very 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 – 255.742 -36.927 1.036 1.19 -2.412 -0.534
Hunt & Reffert 2024 255.762 -36.908 1.023 1.223 -2.429 -12.753
Cavallo et al. 2024 255.758 -36.944 1.018 – – –
Hunt & Reffert 2023 255.762 -36.908 1.023 1.223 -2.429 -12.753

💡 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 – – – – – 152* – –
Cavallo et al. 2024 1.00 1.31 – 7 -0.160 – – –
Hunt & Reffert 2023 0.93 1.07 0.74 13 – – – –

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

Visualization

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