FSR 1387

(SAI 89; MWSC 1486)

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0.21 UTI
0.0
CN
0.36
Cdens
0.5
CC3
0.1
Clit
1.0
Cdup
Core radius and density 1.4 [pc], 1.8 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.36 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.1 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
FSR 1387 is a sparse, loose object of intermediate C3 quality. Its parallax locates it at a large* distance, below the mid-plane, affected by moderate extinction. It is catalogued as an old cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 7 years.

(*): The parallax distance estimate (~5.41 kpc) differs significantly from the median photometric distance (~1.26 kpc).

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

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.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 126.103 -39.94 0.185 -2.595 3.282 207.082
Bica et al. 2019 126.108 -39.94 – – – –
Dib et al. 2018 126.129 -39.905 – – – –
Joshi et al. 2016 126.129 -39.905 – – – –
Glushkova et al. 2010 126.105 -39.936 – – – –
Froebrich et al. 2007 126.108 -39.922 – – – –

💡 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– 1.26 2.86 – 1047 – – – –
Dib et al. 2018 1.26 – – 1047 – – – –
Joshi et al. 2016 1.26 1.97 – 1047 – – – –
Glushkova et al. 2010 2.31 3.75 – 631 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3174 80.0 126.11 -39.94 0.18 -2.6 3.24 207.08 0.04

💡 Note: The % column shows the percentage of members that FSR 1387 shares with each listed object.

Visualization

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