HSC 2761

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0.38 UTI
0.76
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.68
Cdup
Radius (P>50% members) 3.2 [arcmin]
  • CN 0.76 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.68 Likely unique

Overview

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HSC 2761 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, young 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 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 – 245.3 -50.936 0.245 -3.014 -3.84 -29.69
Hunt & Reffert 2024 245.303 -50.933 0.235 -3.022 -3.831 -20.191
Cavallo et al. 2024 245.213 -50.927 0.237 – – –
Hunt & Reffert 2023 245.303 -50.933 0.235 -3.022 -3.831 -20.191

💡 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 – – – – – 1609* – –
Cavallo et al. 2024 5.13 4.80 – 7 0.040 – – –
Hunt & Reffert 2023 3.80 4.61 3.11 61 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
DBSB 100 32.1 245.11 -50.91 0.21 -2.96 -3.68 -17.68 0.7

💡 Note: The % column shows the percentage of members that HSC 2761 shares with each listed object.

Visualization

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