HSC 2661

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0.53 UTI
0.64
CN
1.0
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 3.8 [arcmin]
  • CN 0.64 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2661 is a moderately populated, very dense object of very 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, young cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.

Distant Very high extinction Massive Near-solar metallicity Young

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 – 222.379 -59.766 0.302 -4.682 -2.699 18.529
Hunt & Reffert 2024 222.377 -59.749 0.294 -4.714 -2.733 28.025
Cavallo et al. 2024 222.327 -60.0 0.294 – – –
Hunt & Reffert 2023 222.377 -59.749 0.294 -4.714 -2.733 28.025

💡 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 – – – – – 1240* – –
Cavallo et al. 2024 3.18 5.28 – 11 0.430 – – –
Hunt & Reffert 2023 3.17 5.69 3.05 58 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4359 62.0 222.38 -59.76 0.29 -4.63 -2.68 64.53 0.03

💡 Note: The % column shows the percentage of members that HSC 2661 shares with each listed object.

Visualization

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