Barkhatova 2

(MWSC 3552)

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0.26 UTI
0.0
CN
0.06
Cdens
0.25
CC3
0.5
Clit
1.0
Cdup
Stellar density (N50/rad) 0.3 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.06 Very loose
  • CC3 0.25 Low quality
  • Clit 0.5 Moderately studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Barkhatova 2 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate* distance, below the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~3.63 kpc) differs significantly from the median photometric distance (~1.31 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.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 325.855 51.048 0.275 -4.188 -4.305 -65.986
Just et al. 2023 325.911 51.066 – – – –
Loktin & Popova 2017 325.905 51.071 – -1.976 -3.402 –
Kharchenko et al. 2016 325.911 51.066 – – – –
Dias et al. 2014 325.908 51.071 – -0.53 -1.46 –
Kharchenko et al. 2013 325.917 51.07 – -2.2 -3.53 –
Kharchenko et al. 2012 325.917 51.07 – -2.2 -3.53 –
Bukowiecki et al. 2011 325.879 51.059 – – – –
Dias et al. 2002 325.908 51.071 – -0.53 -1.46 –

💡 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– 1.315 1.535 – 429 – 288 – –
Just et al. 2023 – – – 429 – 23 – –
Loktin & Popova 2017 1.53 2.14 – 7 – – – –
Kharchenko et al. 2016 1.10 0.93 – 429 – – – –
Kharchenko et al. 2013 1.10 0.93 – 429 – – – –
Bukowiecki et al. 2012 – – – – – 552 – –
Kharchenko et al. 2012 1.10 0.93 – 429 – – – –
Bukowiecki et al. 2011 2.27(1) 2.33 – 7 – – – –
Dias et al. 2002 1.68 2.39 – 7 – – – –

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

Visualization

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