HSC 2801

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0.34 UTI
0.61
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.65
Cdup
Radius (P>50% members) 1.5 [arcmin]
  • CN 0.61 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.65 Likely unique

Overview

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HSC 2801 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a large 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 is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Distant High extinction Massive Near-solar metallicity Intermediate age

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 – 248.428 -45.808 0.199 -2.791 -3.496 -30.105
Hunt & Reffert 2024 248.419 -45.813 0.2 -2.791 -3.492 -30.976
Cavallo et al. 2024 248.431 -45.811 0.199 – – –
Hunt & Reffert 2023 248.419 -45.813 0.2 -2.791 -3.492 -30.976

💡 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 – – – – – 2960* – –
Cavallo et al. 2024 3.98 4.62 – 302 0.440 – – –
Hunt & Reffert 2023 4.31 4.80 2.49 160 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0664 34.7 248.42 -45.81 0.17 -2.8 -3.47 -31.02 0.38

💡 Note: The % column shows the percentage of members that HSC 2801 shares with each listed object.

Visualization

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