FSR 1712

(MWSC 2332; GLIMPSE 68; Mercer 68)

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0.15 UTI
0.0
CN
0.25
Cdens
0.12
CC3
0.31
Clit
0.76
Cdup
Radius (P>50% members) 7.9 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.25 Loose
  • CC3 0.12 Very low quality
  • Clit 0.31 Poorly studied
  • Cdup 0.76 Very likely unique

Overview

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FSR 1712 is a sparse, loose object of very low C3 quality. Its parallax locates it at a relatively close* distance, near the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~1.82 kpc) differs significantly from the median photometric distance (~1.14 kpc).

Note: This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry. See table with shared members information.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.76) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close Moderate extinction Intermediate age

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 238.711 -52.478 0.549 -5.654 -5.486 –
Just et al. 2023 238.668 -52.479 – – – –
Bica et al. 2019 238.694 -52.528 – – – –
Kharchenko et al. 2016 238.668 -52.479 – – – –
Kharchenko et al. 2013 238.68 -52.48 – -4.57 -2.67 –
Froebrich et al. 2007 238.692 -52.502 – – – –

💡 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
Just et al. 2023 – – – 398 – 76 – –
Kharchenko et al. 2016 1.14 2.13 – 398 – – – –
Kharchenko et al. 2013 1.14 2.13 – 398 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
MCM 68 24.0 238.66 -52.54 0.37 -5.73 -5.23 – 0.05

💡 Note: The % column shows the percentage of members that FSR 1712 shares with each listed object.

Visualization

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