HSC 79

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0.24 UTI
0.0
CN
1.0
Cdens
0.25
CC3
0.0
Clit
0.96
Cdup
Radius (P>50% members) 2.4 [arcmin]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.96 Unique

Overview

â„šī¸
HSC 79 is a sparse, very 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 very metal-poor, young cluster (see Parameters). It was recently reported in the literature.

Note: This is a unique object, which shares a very 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=0.96) 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 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 – 270.06 -24.291 0.478 0.092 -1.179 92.364
Hunt & Reffert 2024 270.068 -24.288 0.476 0.078 -1.168 92.365
Cavallo et al. 2024 270.122 -24.308 0.475 – – –
Hunt & Reffert 2023 270.068 -24.288 0.476 0.078 -1.168 92.365

💡 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 – – – – – 332* – –
Cavallo et al. 2024 2.91 2.88 – 141 -1.260 – – –
Hunt & Reffert 2023 1.94 2.55 2.10 7 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4102 76.0 270.06 -24.29 0.47 0.09 -1.15 37.84 0.07
Ryu 596 4.0 270.22 -24.23 0.39 0.06 -1.42 25.14 0.22

💡 Note: The % column shows the percentage of members that HSC 79 shares with each listed object.

Visualization

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