HSC 2914

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0.21 UTI
0.31
CN
0.5
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 9.7 [arcmin]
  • CN 0.31 Poorly populated
  • Cdens 0.5 Moderately dense
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2914 is a poorly populated, moderately dense object of low C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a very metal-poor, intermediate-age cluster (see Parameters). It was recently reported in the literature.

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

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close Moderate extinction Very metal-poor Intermediate age

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 – 259.723 -33.554 0.804 2.358 -1.837 55.595
Hunt & Reffert 2024 259.681 -33.549 0.815 2.325 -1.859 –
Cavallo et al. 2024 259.681 -33.556 0.812 – – –
Hunt & Reffert 2023 259.681 -33.549 0.815 2.325 -1.859 –

💡 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 – – – – – 202* – –
Cavallo et al. 2024 2.27 1.42 – 295 -1.290 – – –
Hunt & Reffert 2023 1.21 1.59 1.14 75 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3580 93.5 259.72 -33.57 0.8 2.37 -1.83 55.59 0.02

💡 Note: The % column shows the percentage of members that HSC 2914 shares with each listed object.

Visualization

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