FSR 1197

(MWSC 1015)

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0.60 UTI
0.74
CN
0.62
Cdens
0.75
CC3
0.45
Clit
1.0
Cdup
Stellar density (N50/rad) 3.1 [N/pc2]
  • CN 0.74 Moderately populated
  • Cdens 0.62 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.45 Poorly studied
  • Cdup 1.0 Unique

Overview

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FSR 1197 is a moderately populated, moderately dense object of high C3 quality. Its parallax locates it at a close* distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, old cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~0.85 kpc) differs significantly from the median photometric distance (~1.24 kpc).

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 99999– 103.671 -13.861 1.175 -3.039 -0.716 25.707
Hunt & Reffert 2024 103.591 -13.748 1.151 -3.046 -0.709 26.929
Cavallo et al. 2024 103.596 -13.882 1.165 – – –
Hunt & Reffert 2023 103.591 -13.748 1.151 -3.046 -0.709 26.929
Just et al. 2023 103.618 -13.657 – – – –
Bica et al. 2019 103.63 -13.656 – – – –
Kharchenko et al. 2016 103.618 -13.657 – – – –
Kharchenko et al. 2013 103.624 -13.658 – 2.36 -2.17 –
Froebrich et al. 2007 103.625 -13.658 – – – –

💡 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] Bfrac BSS
UCC 99999– 1.24 0.83 0.64 1000 0.120 126 – –
Hunt & Reffert 2024 – – – – – 198(1) – –
Cavallo et al. 2024 0.85 0.37 – 182 0.120 – – –
Hunt & Reffert 2023 0.81 0.14 0.64 146 – – – –
Just et al. 2023 – – – 1000 – 53 – –
Kharchenko et al. 2016 1.63 1.29 – 1000 – – – –
Kharchenko et al. 2013 1.63 1.29 – 1000 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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