C1331 622

(MWSC 2137)

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0.23 UTI
0.0
CN
0.02
Cdens
0.38
CC3
0.38
Clit
1.0
Cdup
Stellar density (N50/rad) 0.1 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.02 Very loose
  • CC3 0.38 Low quality
  • Clit 0.38 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
C1331 622 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large* distance, near the mid-plane, affected by low extinction. It is catalogued as an old cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~5.71 kpc) differs significantly from the median photometric distance (~1.08 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– 203.611 -62.353 0.175 -6.959 -1.269 -22.097
Just et al. 2023 203.644 -62.414 – – – –
Kharchenko et al. 2016 203.644 -62.414 – – – –
Dias et al. 2014 203.55 -62.417 – -1.59 -4.43 -35.0
Kharchenko et al. 2013 203.655 -62.417 – -7.61 0.93 –
Morales et al. 2013 203.55 -62.417 – – – –
Bukowiecki et al. 2011 203.642 -62.458 – – – –
Dias et al. 2002 203.55 -62.417 – -1.59 -4.43 -35.0

💡 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– 1.08 0.84 – 1778 – 326 – –
Just et al. 2023 – – – 1778 – 35 – –
Kharchenko et al. 2016 1.08 0.84 – 1778 – – – –
Kharchenko et al. 2013 1.08 0.84 – 1778 – – – –
Morales et al. 2013 1.09 – – 63 – – – –
Bukowiecki et al. 2012 – – – – – 617 – –
Bukowiecki et al. 2011 1.28(1) 1.21 – 63 – – – –
Dias et al. 2002 0.82 0.71 – – – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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