FSR 1435

(SAI 98; MWSC 1604)

Click to load Aladin Lite
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

â„šī¸
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

Cavallo et al. (2024)
Bronze sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 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 – – – –
Cavallo et al. 2024 134.19 -43.751 0.461 – – –
Hunt & Reffert 2023 134.261 -43.757 0.459 -3.874 2.774 41.933
Just et al. 2023 134.268 -43.762 – – – –
Cantat-Gaudin et al. 2020 134.218 -43.757 0.436 -3.9 2.732 –
Cantat-Gaudin & Anders 2020 134.218 -43.757 0.436 -3.9 2.732 –
Soubiran et al. 2018 134.218 -43.757 – – – 29.17
Bica et al. 2019 134.266 -43.763 – – – –
Cantat-Gaudin et al. 2018 134.218 -43.757 0.436 -3.9 2.732 –
Kharchenko et al. 2016 134.268 -43.762 – – – –
Kharchenko et al. 2013 134.272 -43.765 – -9.37 12.58 –
Glushkova et al. 2010 134.262 -43.761 – – – –
Froebrich et al. 2007 134.258 -43.758 – – – –

💡 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 – – – – – 547* – –
Celli et al. 2024 – – – 1 – 402 – –
Cavallo et al. 2024 2.54 3.83 – 316 0.340 – – –
Hunt & Reffert 2023 2.02 4.24 2.80 179 – – – –
Just et al. 2023 – – – 1 – 337 – –
Cantat-Gaudin & Anders 2020 2.15 – – – – – – –
Soubiran et al. 2018 2.15 – – – – – – –
Cantat-Gaudin et al. 2018 2.15 – – – – – – –
Kharchenko et al. 2016 1.30 8.07 – 1 – – – –
Kharchenko et al. 2013 1.30 8.07 – 1 – – – –
Glushkova et al. 2010 1.13 3.29 – 5623 – – – –

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

Visualization

â„šī¸