HSC 273

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0.05 UTI
0.0
CN
0.06
Cdens
0.25
CC3
0.0
Clit
0.88
Cdup
Radius (P>50% members) 6.5 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.06 Very loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.88 Very likely unique

Overview

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HSC 273 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate* distance, below the mid-plane, affected by high extinction. It is catalogued as a massive, metal-poor, young cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~4.25 kpc) differs significantly from the median photometric distance (~3.12 kpc).

Note: This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry. See table with shared members information.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.88) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Distant High extinction Massive Metal-poor Young

Cavallo et al. (2024)
Bronze sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 281.082 -5.454 0.235 -1.205 -3.096 38.573
Hunt & Reffert 2024 281.107 -5.445 0.246 -1.204 -3.11 38.856
Cavallo et al. 2024 281.191 -5.451 0.246 – – –
Hunt & Reffert 2023 281.107 -5.445 0.246 -1.204 -3.11 38.856

💡 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 – – – – – 2022* – –
Cavallo et al. 2024 2.59 3.88 – 26 -0.860 – – –
Hunt & Reffert 2023 3.65 3.32 2.85 23 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2662 12.0 281.27 -5.46 0.26 -1.33 -3.2 55.52 0.4

💡 Note: The % column shows the percentage of members that HSC 273 shares with each listed object.

Visualization

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