FSR 1701

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0.14 UTI
0.0
CN
0.03
Cdens
0.62
CC3
0.03
Clit
1.0
Cdup
Core radius and density 4.5 [pc], 0.1 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.03 Very loose
  • CC3 0.62 Intermediate quality
  • Clit 0.03 Rarely studied
  • Cdup 1.0 Unique

Overview

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FSR 1701 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane. It is catalogued as an intermediate-age cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 8 years.

(*): The parallax distance estimate (~4.76 kpc) differs significantly from the median photometric distance (~1.50 kpc).

âš 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

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 231.879 -57.044 0.21 -5.194 -3.411 -62.933
Dib et al. 2018 232.11 -56.997 – – – –
Morales et al. 2013 232.117 -57.02 – – – –
Froebrich et al. 2007 232.117 -57.02 – – – –

💡 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– 1.5 – – 251 – – – –
Dib et al. 2018 1.50 – – 251 – – – –

Visualization

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