HSC 2629

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0.00 UTI
0.0
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.0
Cdup
Radius (P>50% members) 0.8 [arcmin]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.0 Very likely duplicate

Overview

â„šī¸
HSC 2629 is a sparse, 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, metal-rich, intermediate-age cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Distant Very high extinction Massive Metal-rich Intermediate age

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 – 210.686 -61.956 0.364 -7.666 -2.137 -36.745
Hunt & Reffert 2024 210.688 -61.953 0.391 -7.663 -2.128 –
Cavallo et al. 2024 210.694 -61.948 0.382 – – –
Hunt & Reffert 2023 210.688 -61.953 0.391 -7.663 -2.128 –

💡 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 – – – – – 1643* – –
Cavallo et al. 2024 3.73 4.68 – 115 0.900 – – –
Hunt & Reffert 2023 2.37 6.51 2.18 90 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UFMG 54 100.0 210.69 -61.96 0.29 -7.65 -2.15 -36.72 0.66

💡 Note: The % column shows the percentage of members that HSC 2629 shares with each listed object.

Visualization

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