Platais 6

(HIP 29713 Group; MWSC 821)

Click to load Aladin Lite
0.30 UTI
0.0
CN
0.07
Cdens
0.25
CC3
0.6
Clit
1.0
Cdup
Radius (P>50% members) 120.1 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.07 Very loose
  • CC3 0.25 Low quality
  • Clit 0.6 Moderately studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Platais 6 is a sparse, very loose object of low C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a massive, near-solar metallicity, young cluster (see Parameters). It is moderately studied in the literature.
Very close Low extinction Massive 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 – 94.102 2.929 4.275 -0.844 -12.875 31.861
Zhang et al. 2024 94.896 5.301 – – – –
Cavallo et al. 2024 95.039 1.5 4.406 – – –
Hunt & Reffert 2023 94.896 5.301 4.407 -1.096 -12.679 29.134
Bica et al. 2019 93.855 3.852 – – – –
Dias et al. 2014 93.858 3.845 – -0.45 -2.6 –
Gozha et al. 2012 93.858 3.845 – – – –
Piskunov et al. 2008 93.854 3.919 – – – –
Kharchenko et al. 2007 93.85 3.85 – 1.57 – 13.1
van den Bergh 2006 93.858 3.845 – – – –
Kharchenko et al. 2005 93.85 3.92 – -4.45 -4.27 26.0

💡 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 – – – – 0.098* – – –
Cavallo et al. 2024 0.23 0.22 – 22 -0.040 – – –
Hunt & Reffert 2023 0.23 0.15 0.57 48 – – – –
Gozha et al. 2012 0.35 – – 60 – 2455 – –
Piskunov et al. 2008 0.35 0.00 – 62 – – – –
van den Bergh 2006 0.35 – – 60 – – – –
Kharchenko et al. 2005 0.35 0.00 – 62 – – – –

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

Visualization

â„šī¸