FSR 0435

(MWSC 3736)

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0.44 UTI
0.31
CN
0.27
Cdens
0.5
CC3
0.55
Clit
1.0
Cdup
Radius (P>50% members) 16.6 [arcmin]
  • CN 0.31 Poorly populated
  • Cdens 0.27 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.55 Moderately studied
  • Cdup 1.0 Unique

Overview

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FSR 0435 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a low-mass, near-solar metallicity, intermediate-age cluster (see Parameters). It is moderately studied in the literature.
Close Moderate extinction Low mass Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 352.883 59.792 1.009 -1.077 -2.034 -20.872
Hunt & Reffert 2024 352.882 59.78 0.995 -1.051 -2.016 -15.436
Cavallo et al. 2024 352.926 59.811 0.998 – – –
Hunt & Reffert 2023 352.882 59.78 0.995 -1.051 -2.016 -15.436
Just et al. 2023 352.799 59.771 – – – –
Kharchenko et al. 2016 352.799 59.771 – – – –
Kharchenko et al. 2013 352.807 59.775 – -2.33 -0.71 –
Kharchenko et al. 2012 352.807 59.775 – -2.33 -0.71 –
Froebrich et al. 2007 352.792 59.786 – – – –
Dias et al. 2002 352.792 59.786 – -2.33 -0.71 –

💡 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 – – – – – 56* – –
Cavallo et al. 2024 1.06 2.28 – 30 0.090 – – –
Hunt & Reffert 2023 0.95 2.02 1.01 58 – – – –
Just et al. 2023 – – – 224 – 18 – –
Kharchenko et al. 2016 0.81 1.65 – 224 – – – –
Kharchenko et al. 2013 0.81 1.65 – 224 – – – –
Kharchenko et al. 2012 0.81 1.65 – 224 – – – –
Dias et al. 2002 0.81 1.65 – 224 – – – –

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

Visualization

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