RSG9y

(RSG9o; TRSG 9; Teutsch J0450.9+5209)

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0.59 UTI
0.47
CN
1.0
Cdens
0.75
CC3
0.38
Clit
1.0
Cdup
Radius (P>50% members) 23.3 [arcmin]
  • CN 0.47 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.38 Poorly studied
  • Cdup 1.0 Unique

Overview

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RSG9y is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

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

Very close Moderate extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

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

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 72.608 52.295 3.309 9.293 -16.972 13.354
Wei et al. 2025 72.621 52.421 3.333 9.163 -17.074 –
Zhang et al. 2024 72.57 52.264 – – – –
Cavallo et al. 2024 72.974 52.194 3.325 – – –
Hunt & Reffert 2023 72.57 52.264 3.31 9.126 -16.951 13.829
Bica et al. 2019 72.722 52.156 – – – –
Roser et al. 2016 72.75 52.23 – 8.39 -15.23 –

💡 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
Wei et al. 2025 0.50 1.41 – 288 0.250 118 0.31 –
Zhang et al. 2024 – – – – 0.042* – – –
Cavallo et al. 2024 0.31 1.26 – 186 0.260 – – –
Hunt & Reffert 2023 0.29 0.78 1.92 283 – – – –
Roser et al. 2016 0.22 0.16* – 32* – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1191 95.7 72.51 52.29 3.31 9.32 -16.97 13.24 0.05

💡 Note: The % column shows the percentage of members that RSG9y shares with each listed object.

Visualization

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