FSR 1115

(MWSC 739)

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0.56 UTI
0.27
CN
1.0
Cdens
0.75
CC3
0.4
Clit
1.0
Cdup
Stellar density (N50/rad) 195.7 [N/pc2]
  • CN 0.27 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.4 Poorly studied
  • Cdup 1.0 Unique

Overview

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FSR 1115 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by very 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 poorly studied in the literature.

Palma et al. (2025)
Part of multiple system G88, along with FSR_1117 and Theia_15.

Cavallo et al. (2024)
Wood 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– 92.058 -9.585 1.175 -2.628 0.975 68.954
Hunt & Reffert 2024 92.056 -9.58 1.173 -2.682 0.934 68.941
Cavallo et al. 2024 91.986 -9.519 1.178 – – –
Hunt & Reffert 2023 92.056 -9.58 1.173 -2.682 0.934 68.941
Just et al. 2023 92.049 -9.579 – – – –
Kharchenko et al. 2016 92.049 -9.579 – – – –
Kharchenko et al. 2013 92.055 -9.58 – 0.55 3.41 –
Froebrich et al. 2007 92.067 -9.596 – – – –

💡 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– 1.07 5.24 2.23 8 0.020 63 – –
Hunt & Reffert 2024 – – – – – 94(1) – –
Cavallo et al. 2024 2.58 2.54 – 2399 0.020 – – –
Hunt & Reffert 2023 0.82 3.19 2.23 17 – – – –
Just et al. 2023 – – – 8 – 32 – –
Kharchenko et al. 2016 1.07 7.29 – 8 – – – –
Kharchenko et al. 2013 1.07 7.29 – 8 – – – –

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

Visualization

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