NGC 3603
0.86
UTI
0.9
CN
1.0
Cdens
0.75
CC3
0.82
Clit
1.0
Cdup
Radius (P>50% members)
1.1 [arcmin]
- CN 0.9 Very rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.82 Well-studied
- Cdup 1.0 Unique
Overview
NGC 3603 is a very rich, very dense object of high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by high extinction. It is catalogued as a very massive, near-solar metallicity, very young cluster, but with a large variance across recent sources for the distance and age parameters (see Parameters). It is well-studied in the literature.
Very distant
High extinction
Very massive
Near-solar metallicity
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 168.795 | -61.263 | 0.107 | -5.578 | 1.96 | 46.083 |
| Hunt & Reffert | 2024 | 168.79 | -61.261 | 0.115 | -5.612 | 1.988 | -24.616 |
| Celli et al. | 2024 | 168.795 | -61.259 | â | â | â | â |
| Cavallo et al. | 2024 | 168.774 | -61.248 | 0.115 | â | â | â |
| Hunt & Reffert | 2023 | 168.79 | -61.261 | 0.115 | -5.612 | 1.988 | -24.616 |
| Jaehnig et al. | 2021 | 168.798 | -61.258 | 0.106 | -5.52 | 1.959 | â |
| Rain et al. | 2021 | 168.795 | -61.259 | 0.076 | -5.543 | 1.961 | â |
| Cantat-Gaudin et al. | 2020 | 168.795 | -61.259 | 0.076 | -5.543 | 1.961 | â |
| Cantat-Gaudin & Anders | 2020 | 168.795 | -61.259 | 0.076 | -5.543 | 1.961 | â |
| Soubiran et al. | 2018 | 168.795 | -61.259 | â | â | â | 28.17 |
| Cantat-Gaudin et al. | 2018 | 168.795 | -61.259 | 0.076 | -5.543 | 1.961 | â |
| Loktin & Popova | 2017 | 168.78 | -61.26 | â | -5.76 | 0.28 | 23.0 |
| Dias et al. | 2014 | 168.779 | -61.26 | â | -1.77 | -2.73 | â |
| van den Bergh | 2006 | 168.788 | -61.271 | â | â | â | â |
| Dias et al. | 2002 | 168.779 | -61.26 | â | -5.76 | 0.28 | â |
| Dambis | 1999 | 168.788 | -61.271 | â | â | â | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | â | â | â | â | â | 8098* | â | â |
| Celli et al. | 2024 | â | â | â | 1 | â | 4808 | â | â |
| Cavallo et al. | 2024 | 2.34 | 4.39 | â | 74 | 0.320 | â | â | â |
| Hunt & Reffert | 2023 | 8.70 | 4.65 | 2.69 | 7 | â | â | â | â |
| Jaehnig et al. | 2021 | 9.52* | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 9.49 | 4.12 | â | 1 | â | â | â | 0 |
| Cantat-Gaudin & Anders | 2020 | 9.49 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 9.49 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 9.49 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 3.80 | 4.19 | â | 7 | â | â | â | â |
| van den Bergh | 2006 | 3.63 | 4.15 | â | 7 | â | â | â | â |
| Dias et al. | 2002 | 6.90 | 4.15 | â | 1 | â | â | â | â |
| Dambis | 1999 | 9.46 | 4.40 | â | 3 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Silver sample.