Sh2-287C

(MWSC 1052)

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0.12 UTI
0.0
CN
0.21
Cdens
0.25
CC3
0.06
Clit
1.0
Cdup
Core radius and density 1.1 [pc], 1.0 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.21 Very loose
  • CC3 0.25 Low quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Sh2-287C 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 low-mass, very young cluster (see Parameters). It is rarely studied in the literature.

(*): The parallax distance estimate (~2.22 kpc) differs significantly from the median photometric distance (~3.34 kpc).

Note: This object shares a significant percentage of members with 4 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.

Bica et al. (2003)
Classified as infrared cluster (IRC).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 104.85 -4.703 0.45 -1.608 0.763 48.19
Just et al. 2023 104.896 -4.665 – – – –
Kharchenko et al. 2016 104.896 -4.665 – – – –
Kharchenko et al. 2013 104.902 -4.667 – -0.01 1.96 –
Bica et al. 2003 104.899 -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– 3.34 3.61 – 8 – 41 – –
Just et al. 2023 – – – 8 – 41 – –
Kharchenko et al. 2016 3.34 3.61 – 8 – – – –
Kharchenko et al. 2013 3.34 3.61 – 8 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 1723 52.0 104.85 -4.74 0.43 -1.49 0.69 62.26 0.04
S 287 C 44.0 104.88 -4.74 0.44 -1.46 0.6 62.26 0.06
HSC 1721 20.0 104.97 -4.52 0.45 -1.89 0.6 – 0.08
BDSB 90 8.0 104.89 -4.81 0.44 -1.49 0.61 62.26 0.18

💡 Note: The % column shows the percentage of members that Sh2-287C shares with each listed object.

Visualization

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