HSC 1248

Click to load Aladin Lite
0.37 UTI
0.35
CN
0.25
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 9.9 [arcmin]
  • CN 0.35 Poorly populated
  • Cdens 0.25 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 1248 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Young

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 – 63.303 43.072 0.548 0.24 -2.742 -24.924
Zhang et al. 2024 63.243 43.053 – – – –
Hunt & Reffert 2024 63.243 43.053 0.535 0.241 -2.717 -22.039
Cavallo et al. 2024 63.331 43.123 0.541 – – –
Hunt & Reffert 2023 63.243 43.053 0.535 0.241 -2.717 -22.039

💡 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 – – – – -0.014* – – –
Hunt & Reffert 2024 – – – – – 214* – –
Cavallo et al. 2024 1.91 1.57 – 26 0.510 – – –
Hunt & Reffert 2023 1.71 1.55 1.29 46 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2928 94.3 63.31 43.12 0.55 0.23 -2.74 -17.26 0.12

💡 Note: The % column shows the percentage of members that HSC 1248 shares with each listed object.

Visualization

â„šī¸