RSG1
(Alessi 96; OCSN 255)
0.96
UTI
0.82
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
43.5 [arcmin]
- CN 0.82 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
RSG1 is a rich, very dense object of very high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is very well-studied in the literature.
Very close
Low extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 75.554 | 37.481 | 3.027 | 0.688 | -12.384 | 13.507 |
| Li et al. | 2025 | 75.508 | 37.475 | 3.001 | 0.77 | -12.33 | â |
| Wei et al. | 2025 | 75.557 | 37.434 | 3.034 | 0.657 | -12.389 | â |
| Almeida et al. | 2025 | 75.525 | 37.481 | â | â | â | â |
| Alfonso et al. | 2024 | 75.483 | 37.525 | 2.997 | 0.75 | -12.411 | â |
| Zhang et al. | 2024 | 75.485 | 37.488 | â | â | â | â |
| Hunt & Reffert | 2024 | 75.485 | 37.488 | 3.053 | 0.971 | -12.561 | 11.589 |
| Cavallo et al. | 2024 | 74.195 | 38.441 | 3.065 | â | â | â |
| Hunt & Reffert | 2023 | 75.485 | 37.488 | 3.053 | 0.971 | -12.561 | 11.589 |
| Almeida et al. | 2023 | 75.554 | 37.499 | â | â | â | â |
| Qin et al. | 2023 | 75.55 | 37.52 | 3.04 | 0.74 | -12.42 | 14.28 |
| He et al. | 2022 | 75.511 | 37.508 | 3.035 | 0.703 | -12.423 | â |
| Tarricq et al. | 2022 | 75.529 | 37.481 | 3.037 | 0.703 | -12.419 | â |
| Dias et al. | 2021 | 75.525 | 37.481 | 3.002 | 0.768 | -12.368 | 13.406 |
| Cantat-Gaudin et al. | 2020 | 75.508 | 37.475 | 3.001 | 0.77 | -12.33 | â |
| Cantat-Gaudin & Anders | 2020 | 75.508 | 37.475 | 3.001 | 0.77 | -12.33 | â |
| Soubiran et al. | 2018 | 75.508 | 37.475 | â | â | â | 14.69 |
| Bica et al. | 2019 | 75.569 | 37.558 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 75.508 | 37.475 | 3.001 | 0.77 | -12.33 | â |
| Roser et al. | 2016 | 75.57 | 37.56 | â | 0.2 | -12.32 | â |
đĄ 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 |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 0.32 | 0.68 | â | 106 | 0.042 | â | â | â |
| Wei et al. | 2025 | 0.49 | 1.20 | â | 50 | -0.250 | 146 | 0.19 | â |
| Almeida et al. | 2025 | 0.33 | 0.59 | â | 303 | â | 144 | â | â |
| Alfonso et al. | 2024 | 0.35 | 0.53 | â | 122 | 0.063 | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | 0.003* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 193* | â | â |
| Cavallo et al. | 2024 | 0.33 | 1.02 | â | 78 | 0.010 | â | â | â |
| Hunt & Reffert | 2023 | 0.32 | 0.36 | 1.14 | 207 | â | â | â | â |
| Almeida et al. | 2023 | 0.31 | 0.74 | â | 242 | -0.101 | 179* | 0.50 | â |
| Qin et al. | 2023 | 0.45 | 0.78 | â | 79 | â | â | â | â |
| He et al. | 2022 | â | 0.90 | â | 112 | â | â | â | â |
| Tarricq et al. | 2022 | 0.34 | â | â | 120 | â | â | â | â |
| Dias et al. | 2021 | 0.33 | 0.59 | â | 303 | 0.063 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.35 | 0.53 | â | 123 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.33 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 0.33 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.33 | â | â | â | â | â | â | â |
| Roser et al. | 2016 | 0.32 | 0.74* | â | 126* | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit. Silver sample.
Cavallo et al. (2024)
Gold sample.