FSR 0035

(MWSC 2797)

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0.15 UTI
0.0
CN
0.04
Cdens
0.25
CC3
0.23
Clit
1.0
Cdup
Nm (P>50%) 17
Core radius and density 1.3 [pc], 0.2 [pc-2]
C3 classification DB
  • CN 0.0 Sparse
  • Cdens 0.04 Very loose
  • CC3 0.25 Low quality
  • Clit 0.23 Rarely studied
  • Cdup 1.0 Unique
đŸ“Ĩ Members 📊 Colab đŸ”Ŧ Bayestar19 MOCAMOCA 🔍 CDS 🔍 Simbad 🔍 CDS (Îą, δ) 🔍 Simbad (Îą, δ)

Overview
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FSR 0035 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a very young cluster (see Parameters). It is rarely studied in the literature.

⚠ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Morales et al. (2013)
Classified as morphological type 'OC2' (totally exposed cluster without correlation with ATLASGAL emission). Morphological flag: exposed cluster, without submm emission.

Data
🔍 Search references for FSR 0035 in: SciX Simbad
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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 271.138 -20.168 0.327 -0.059 -2.123 9.921
Just et al. 2023 271.064 -20.179 – – – –
Bica et al. 2019 271.072 -20.189 – – – –
Sampedro et al. 2017 271.067 -20.191 – -1.12 -1.31 –
Kharchenko et al. 2016 271.064 -20.179 – – – –
Dias et al. 2014 271.067 -20.191 – -12.14 -13.66 –
Kharchenko et al. 2013 271.072 -20.178 – 2.79 -3.79 –
Morales et al. 2013 271.067 -20.191 – – – –
Froebrich et al. 2007 271.067 -20.191 – – – –
Dias et al. 2002 271.067 -20.191 – 2.79 -3.79 –

💡 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– 2.52 3.81 – 4 – 133 – –
Just et al. 2023 – – – 4 – 133 – –
Kharchenko et al. 2016 2.52 3.81 – 4 – – – –
Kharchenko et al. 2013 2.52 3.81 – 4 – – – –
Dias et al. 2002 2.52 3.81 – 4 – – – –

Visualization
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FSR 0035 UCC
Galactocentric position diagram