NGC 2270

(MWSC 971)

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0.29 UTI
0.0
CN
0.02
Cdens
0.12
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members) 9.0 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.02 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.65 Moderately studied
  • Cdup 1.0 Unique

Overview

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NGC 2270 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a large* distance, near 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 (~5.16 kpc) differs significantly from the median photometric distance (~1.40 kpc).

Relatively 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 – 100.991 3.436 0.194 -1.49 0.241 49.074
Just et al. 2023 100.988 3.472 – – – –
Bica et al. 2019 100.984 3.458 – – – –
Loktin & Popova 2017 100.995 3.479 – 1.663 -2.501 40.0
Kharchenko et al. 2016 100.988 3.472 – – – –
Dias et al. 2014 100.987 3.478 – 0.21 -1.99 –
Kharchenko et al. 2013 100.995 3.47 – 1.75 -1.39 40.0
Gozha et al. 2012 100.988 3.478 – – – –
Piskunov et al. 2008 100.993 3.485 – – – –
Kharchenko et al. 2007 100.99 3.48 – 0.32 – 40.0
Piskunov et al. 2007 100.993 3.485 – – – –
Kharchenko et al. 2005 100.99 3.48 – -0.17 -3.12 40.0

💡 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] Bfr BSS
Just et al. 2023 – – – 822 – 97 – –
Loktin & Popova 2017 1.96 0.83 – 209 – – – –
Kharchenko et al. 2016 1.42 0.45 – 822 – – – –
Kharchenko et al. 2013 1.42 0.45 – 822 – – – –
Gozha et al. 2012 1.40 – – 437 – 1479 – –
Piskunov et al. 2008 1.40 0.19 – 437 – 1094* – –
Piskunov et al. 2007 1.40 0.19 – 437 – 347 – –
Kharchenko et al. 2005 1.40 0.19 – 437 – – – –

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

Visualization

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