HSC 1702

Click to load Aladin Lite
0.01 UTI
0.75
CN
0.9
Cdens
1.0
CC3
0.25
Clit
0.01
Cdup
Radius (P>50% members) 4.2 [arcmin]
  • CN 0.75 Rich
  • Cdens 0.9 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 0.01 Very likely duplicate

Overview

â„šī¸
HSC 1702 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low 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.

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 Low 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 – 105.578 -1.856 0.258 -0.908 0.859 66.127
Zhang et al. 2024 105.586 -1.851 – – – –
Hunt & Reffert 2024 105.586 -1.851 0.254 -0.92 0.849 73.025
Cavallo et al. 2024 105.568 -1.857 0.254 – – –
Hunt & Reffert 2023 105.586 -1.851 0.254 -0.92 0.849 73.025

💡 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
Zhang et al. 2024 – – – – -0.146* – – –
Hunt & Reffert 2024 – – – – – 920* – –
Cavallo et al. 2024 3.47 1.03 – 288 0.180 – – –
Hunt & Reffert 2023 3.39 0.48 0.78 535 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 2672 99.0 105.57 -1.85 0.26 -0.91 0.84 68.4 0.25
FoF 373 78.2 105.58 -1.85 0.25 -0.91 0.85 82.74 0.46
OC 0360 24.8 105.58 -1.86 0.25 -0.9 0.86 – 0.0

💡 Note: The % column shows the percentage of members that HSC 1702 shares with each listed object.

Visualization

â„šī¸