HSC 601

Click to load Aladin Lite
0.14 UTI
0.0
CN
0.21
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 26.2 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.21 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 601 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low 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.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Close Low extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 305.312 38.751 1.644 2.141 -1.683 -6.435
Zhang et al. 2024 305.074 38.461 – – – –
Cavallo et al. 2024 306.124 39.148 1.656 – – –
Hunt & Reffert 2023 305.074 38.461 1.659 2.095 -1.56 -9.13

💡 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 – – – – -0.081* – – –
Cavallo et al. 2024 0.61 0.18 – 83 0.500 – – –
Hunt & Reffert 2023 0.58 0.22 0.99 77 – – – –

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

Visualization

â„šī¸