HSC 2911

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0.39 UTI
0.6
CN
0.93
Cdens
1.0
CC3
0.0
Clit
0.77
Cdup
Radius (P>50% members) 11.8 [arcmin]
  • CN 0.6 Moderately populated
  • Cdens 0.93 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.77 Very likely unique

Overview

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HSC 2911 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

Note: This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Low extinction Near-solar metallicity Very 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 – 258.251 -33.286 0.889 1.728 -1.813 7.42
Hunt & Reffert 2024 258.32 -33.267 0.897 1.682 -1.813 -4.117
Cavallo et al. 2024 258.195 -33.363 0.894 – – –
Hunt & Reffert 2023 258.32 -33.267 0.897 1.682 -1.813 -4.117

💡 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 – – – – – 518* – –
Cavallo et al. 2024 0.99 0.73 – 10 0.160 – – –
Hunt & Reffert 2023 1.05 0.64 1.52 8 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 14438 23.2 258.58 -33.16 0.91 1.78 -1.75 3.82 0.29
CWWDL 14435 2.9 258.04 -33.6 0.95 1.46 -1.88 7.3 0.21

💡 Note: The % column shows the percentage of members that HSC 2911 shares with each listed object.

Visualization

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