HSC 2978

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0.27 UTI
0.0
CN
0.97
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 2.7 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.97 Very dense
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2978 is a sparse, very dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, young 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.

Relatively close High extinction Near-solar metallicity 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 – 266.466 -30.296 0.354 -0.298 -2.341 -12.869
Hunt & Reffert 2024 266.486 -30.3 0.354 -0.276 -2.351 -12.871
Cavallo et al. 2024 266.475 -30.288 0.354 – – –
Hunt & Reffert 2023 266.486 -30.3 0.354 -0.276 -2.351 -12.871

💡 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 – – – – – 590* – –
Cavallo et al. 2024 1.95 4.58 – 32 -0.450 – – –
Hunt & Reffert 2023 2.60 4.30 2.67 19 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4284 100.0 266.49 -30.29 0.37 -0.3 -2.34 0.63 0.16

💡 Note: The % column shows the percentage of members that HSC 2978 shares with each listed object.

Visualization

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