HSC 251

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0.49 UTI
0.68
CN
1.0
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 2.9 [arcmin]
  • CN 0.68 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 251 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by very high extinction. It is catalogued as a massive, near-solar metallicity, 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.

Relatively close Very high extinction Massive Near-solar metallicity 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 – 279.347 -6.286 0.334 0.777 -1.033 6.484
Hunt & Reffert 2024 279.332 -6.297 0.338 0.754 -1.053 1.579
Cavallo et al. 2024 279.373 -6.289 0.337 – – –
Hunt & Reffert 2023 279.332 -6.297 0.338 0.754 -1.053 1.579

💡 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 – – – – – 2533* – –
Cavallo et al. 2024 2.62 5.11 – 275 0.140 – – –
Hunt & Reffert 2023 2.57 5.50 3.01 486 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3468 100.0 279.35 -6.28 0.33 0.78 -1.02 9.27 0.17

💡 Note: The % column shows the percentage of members that HSC 251 shares with each listed object.

Visualization

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