FSR 1435
(SAI 98; MWSC 1604)
0.71
UTI
0.6
CN
1.0
Cdens
0.38
CC3
0.79
Clit
1.0
Cdup
Radius (P>50% members)
3.8 [arcmin]
- CN 0.6 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.38 Low quality
- Clit 0.79 Well-studied
- Cdup 1.0 Unique
Overview
FSR 1435 is a moderately populated, very dense object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is well-studied in the literature.
Relatively close
High extinction
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 | 134.241 | -43.756 | 0.452 | -3.858 | 2.761 | 29.684 |
| Hunt & Reffert | 2024 | 134.261 | -43.757 | 0.459 | -3.874 | 2.774 | 41.933 |
| Celli et al. | 2024 | 134.218 | -43.757 | â | â | â | â |
| Cavallo et al. | 2024 | 134.19 | -43.751 | 0.461 | â | â | â |
| Hunt & Reffert | 2023 | 134.261 | -43.757 | 0.459 | -3.874 | 2.774 | 41.933 |
| Just et al. | 2023 | 134.268 | -43.762 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 134.218 | -43.757 | 0.436 | -3.9 | 2.732 | â |
| Cantat-Gaudin & Anders | 2020 | 134.218 | -43.757 | 0.436 | -3.9 | 2.732 | â |
| Soubiran et al. | 2018 | 134.218 | -43.757 | â | â | â | 29.17 |
| Bica et al. | 2019 | 134.266 | -43.763 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 134.218 | -43.757 | 0.436 | -3.9 | 2.732 | â |
| Kharchenko et al. | 2016 | 134.268 | -43.762 | â | â | â | â |
| Kharchenko et al. | 2013 | 134.272 | -43.765 | â | -9.37 | 12.58 | â |
| Glushkova et al. | 2010 | 134.262 | -43.761 | â | â | â | â |
| Froebrich et al. | 2007 | 134.258 | -43.758 | 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 | 547* | â | â |
| Celli et al. | 2024 | â | â | â | 1 | â | 402 | â | â |
| Cavallo et al. | 2024 | 2.54 | 3.83 | â | 316 | 0.340 | â | â | â |
| Hunt & Reffert | 2023 | 2.02 | 4.24 | 2.80 | 179 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 1 | â | 337 | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.15 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 2.15 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.15 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 1.30 | 8.07 | â | 1 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.30 | 8.07 | â | 1 | â | â | â | â |
| Glushkova et al. | 2010 | 1.13 | 3.29 | â | 5623 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Bronze sample.