Collinder 65

(MWSC 540; OCL 474)

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0.31 UTI
0.0
CN
0.01
Cdens
0.25
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members) 8.8 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.01 Very loose
  • CC3 0.25 Low quality
  • Clit 0.65 Moderately studied
  • Cdup 1.0 Unique

Overview

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Collinder 65 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large* distance, well below the mid-plane, affected by low extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~6.58 kpc) differs significantly from the median photometric distance (~0.32 kpc).

Very close Low extinction Intermediate age

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 81.556 16.213 0.152 -0.142 -0.604 75.008
Just et al. 2023 81.517 15.671 – – – –
Bica et al. 2019 81.54 16.226 – – – –
Yen et al. 2018 81.645 15.721 2.77 -0.17 -5.37 –
Loktin & Popova 2017 81.525 16.7 – 1.16 -6.46 21.8
Kharchenko et al. 2016 81.517 15.671 – – – –
Kharchenko et al. 2013 81.525 15.67 – 1.43 -5.62 21.8
Gozha et al. 2012 81.525 16.7 – – – –
Piskunov et al. 2008 81.519 15.7 – – – –
Kharchenko et al. 2007 81.52 16.7 – 2.4 – 19.48
Piskunov et al. 2007 81.519 15.7 – – – –
Kharchenko et al. 2005 81.52 15.7 – 1.16 -6.46 17.4

💡 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] Bfr BSS
Just et al. 2023 – – – 116 – 1346 – –
Yen et al. 2018 0.38 0.10 – 105 – – – –
Loktin & Popova 2017 0.33 0.84 – 631 – – – –
Kharchenko et al. 2016 0.33 0.42 – 116 – – – –
Kharchenko et al. 2013 0.33 0.42 – 116 – – – –
Gozha et al. 2012 0.31 – – 631 – 6607 – –
Piskunov et al. 2008 0.31 0.40 – 26 – 466* – –
Piskunov et al. 2007 0.31 0.40 – 26 – 269 – –
Kharchenko et al. 2005 0.31 0.40 – 26 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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