HSC 2899

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0.26 UTI
0.45
CN
0.37
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 5.4 [arcmin]
  • CN 0.45 Poorly populated
  • Cdens 0.37 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2899 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by 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.

Distant High extinction Massive Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 258.6 -35.922 0.319 -0.94 -2.205 -23.814
Hunt & Reffert 2024 258.556 -35.898 0.336 -0.961 -2.208 -39.894
Cavallo et al. 2024 258.558 -35.945 0.341 – – –
Hunt & Reffert 2023 258.556 -35.898 0.336 -0.961 -2.208 -39.894

💡 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 – – – – – 4111* – –
Cavallo et al. 2024 3.65 4.76 – 603 -0.250 – – –
Hunt & Reffert 2023 2.53 4.97 3.00 982 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3976 77.8 258.75 -35.98 0.28 -0.94 -2.21 -3.49 0.28

💡 Note: The % column shows the percentage of members that HSC 2899 shares with each listed object.

Visualization

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