HSC 2636

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0.10 UTI
0.82
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.17
Cdup
Radius (P>50% members) 130.9 [arcmin]
  • CN 0.82 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.17 Likely duplicate

Overview

â„šī¸
HSC 2636 is a rich, very dense object of very high C3 quality. Its parallax locates it at a very close distance, above the mid-plane, affected by low extinction. It is catalogued as a low-mass, near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

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

Very close Low extinction Low mass 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 – 205.85 -44.769 7.479 -26.275 -19.381 7.744
Hunt & Reffert 2024 204.889 -44.482 7.472 -25.972 -19.412 3.848
Cavallo et al. 2024 206.091 -44.743 7.452 – – –
Hunt & Reffert 2023 204.889 -44.482 7.472 -25.972 -19.412 3.848

💡 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 – – – – – 43* – –
Cavallo et al. 2024 0.13 0.75 – 23 0.110 – – –
Hunt & Reffert 2023 0.13 0.30 0.60 10 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OCSN 317 82.8 205.88 -44.84 7.48 -26.21 -19.41 7.89 0.56

💡 Note: The % column shows the percentage of members that HSC 2636 shares with each listed object.

Visualization

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