HSC 2900

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0.30 UTI
0.25
CN
0.61
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 69.1 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 0.61 Moderately dense
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2900 is a poorly populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
Very close Low extinction Near-solar metallicity Young

Cavallo et al. (2024)
Silver sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 267.024 -40.114 7.038 -7.611 -29.657 -1.371
Cavallo et al. 2024 266.856 -40.141 6.995 – – –
Hunt & Reffert 2023 266.581 -40.053 6.993 -7.775 -29.552 -0.313

💡 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
Cavallo et al. 2024 0.14 1.42 – 48 0.050 – – –
Hunt & Reffert 2023 0.14 0.55 0.47 7 – – – –

Visualization

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