HSC 2842

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0.25 UTI
0.33
CN
0.69
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 5.1 [arcmin]
  • CN 0.33 Poorly populated
  • Cdens 0.69 Moderately dense
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2842 is a poorly populated, moderately dense object of low C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by moderate extinction. It is catalogued as a metal-poor, young cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~2.09 kpc) differs significantly from the median photometric distance (~3.20 kpc).

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Distant Moderate extinction Metal-poor Young

Cavallo et al. (2024)
Wood sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 253.577 -42.783 0.479 -0.191 -1.242 -40.588
Hunt & Reffert 2024 253.584 -42.788 0.47 -0.184 -1.251 -43.534
Cavallo et al. 2024 253.563 -42.79 0.467 – – –
Hunt & Reffert 2023 253.584 -42.788 0.47 -0.184 -1.251 -43.534

💡 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 – – – – – 440* – –
Cavallo et al. 2024 4.39 2.58 – 117 -0.740 – – –
Hunt & Reffert 2023 2.01 2.97 2.61 45 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3614 93.9 253.57 -42.79 0.48 -0.21 -1.24 -46.56 0.02

💡 Note: The % column shows the percentage of members that HSC 2842 shares with each listed object.

Visualization

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