RSG6

(TRSG 6)

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0.03 UTI
0.0
CN
0.07
Cdens
0.25
CC3
0.0
Clit
0.4
Cdup
Core radius and density 2.8 [pc], 0.4 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.07 Very loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.4 Possibly duplicate

Overview

â„šī¸
RSG6 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by low extinction. It is catalogued as a young cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 7 years.

âš ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

(*): The parallax distance estimate (~2.60 kpc) differs significantly from the median photometric distance (~0.35 kpc).

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.4) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 307.444 40.054 0.385 -3.333 -5.494 2.291
Bica et al. 2019 307.491 40.08 – – – –
Roser et al. 2016 307.49 40.08 – 5.86 1.97 –

💡 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] Bfrac BSS
UCC 99999– 0.35 0.13 – 63 – – – –
Roser et al. 2016 0.35 0.13 – 63 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
BDSB 159 60.0 307.34 40.13 0.52 -3.45 -5.49 -9.68 0.17

💡 Note: The % column shows the percentage of members that RSG6 shares with each listed object.

Visualization

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