S 287 C

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0.23 UTI
0.0
CN
0.88
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 4.4 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.88 Dense
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
S 287 C is a sparse, dense object of low C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane. It is catalogued as a low-mass cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 23 years.

(*): The parallax distance estimate (~2.29 kpc) differs significantly from the median photometric distance (~1.40 kpc).

Note: This object shares a significant percentage of members with 3 later reported entries. 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.

Lada & Lada (2003)
Embedded cluster within âˆŧ2 Kpc of the Sun.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 104.88 -4.739 0.437 -1.464 0.603 62.256
Lada & Lada 2003 104.903 -4.673 – – – –

💡 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– 1.4 – – – – 31 – –
Lada & Lada 2003 1.40 – – – – 31 – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 1723 56.0 104.85 -4.74 0.43 -1.49 0.69 62.26 0.08
Sh2 287C 44.0 104.85 -4.7 0.45 -1.61 0.76 48.19 0.09
BDSB 90 24.0 104.89 -4.81 0.44 -1.49 0.61 62.26 0.21

💡 Note: The % column shows the percentage of members that S 287 C shares with each listed object.

Visualization

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