HSC 1631

Click to load Aladin Lite
0.09 UTI
0.0
CN
0.1
Cdens
0.12
CC3
0.25
Clit
0.6
Cdup
Radius (P>50% members) 9.6 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.1 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.25 Poorly studied
  • Cdup 0.6 Likely unique

Overview

â„šī¸
HSC 1631 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (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.

Relatively close Moderate extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 96.982 4.105 0.416 0.393 -2.204 40.599
Zhang et al. 2024 97.046 4.103 – – – –
Hunt & Reffert 2024 97.046 4.103 0.424 0.379 -2.194 40.647
Cavallo et al. 2024 96.81 4.203 0.425 – – –
Hunt & Reffert 2023 97.046 4.103 0.424 0.379 -2.194 40.647

💡 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
Zhang et al. 2024 – – – – -0.212* – – –
Hunt & Reffert 2024 – – – – – 117* – –
Cavallo et al. 2024 2.15 1.45 – 407 0.540 – – –
Hunt & Reffert 2023 2.11 1.64 1.15 109 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1999 40.0 96.73 4.24 0.42 0.38 -2.22 29.25 0.06

💡 Note: The % column shows the percentage of members that HSC 1631 shares with each listed object.

Visualization

â„šī¸