NGC 1513

(MWSC 346; FoF 184)

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1.0 UTI
1.0
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members) 6.7 [arcmin]
  • CN 1.0 Very rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 1.0 Very well-studied
  • Cdup 1.0 Unique

Overview

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NGC 1513 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age, metallicity, and mass parameters (see Parameters). It is very well-studied in the literature.
Relatively close Moderate extinction Massive Near-solar metallicity Intermediate age

Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit.

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 62.47 49.504 0.673 1.306 -3.698 -15.043
Li et al. 2025 62.47 49.504 0.651 1.324 -3.679 –
Almeida et al. 2025 62.475 49.507 – – – –
Zhang et al. 2024 62.472 49.502 – – – –
Hunt & Reffert 2024 62.472 49.502 0.677 1.296 -3.693 -14.938
Cavallo et al. 2024 62.481 49.503 0.678 – – –
Hunt & Reffert 2023 62.472 49.502 0.677 1.296 -3.693 -14.938
Almeida et al. 2023 62.458 49.503 – – – –
Just et al. 2023 62.414 49.509 – – – –
Tarricq et al. 2022 62.476 49.494 0.673 1.318 -3.699 –
Jaehnig et al. 2021 62.465 49.503 0.686 1.3 -3.67 –
Rain et al. 2021 62.47 49.504 0.651 1.324 -3.679 –
Dias et al. 2021 62.475 49.507 0.644 1.32 -3.688 -14.593
Cantat-Gaudin et al. 2020 62.47 49.504 0.651 1.324 -3.679 –
SΓ‘nchez et al. 2020 62.487 49.515 – 1.487 -3.483 –
Cantat-Gaudin & Anders 2020 62.47 49.504 0.651 1.324 -3.679 –
Liu & Pang 2019 62.485 49.498 0.644 1.327 -3.677 –
Soubiran et al. 2018 62.47 49.504 – – – -14.73
Cantat-Gaudin et al. 2018 62.47 49.504 0.651 1.324 -3.679 –
Loktin & Popova 2017 62.49 49.516 – -1.084 -5.576 -15.1
Kharchenko et al. 2016 62.414 49.509 – – – –
Dias et al. 2014 62.487 49.515 – 1.11 -4.66 –
Kharchenko et al. 2013 62.425 49.51 – -1.08 -3.49 -15.1
Gozha et al. 2012 62.488 49.515 – – – –
Kharchenko et al. 2012 62.425 49.51 – -1.08 -3.49 -15.13
van den Bergh 2006 62.65 49.517 – – – –
Dias et al. 2002 62.487 49.515 – 1.11 -4.66 -15.13

πŸ’‘ 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
Li et al. 2025 1.23 1.99 – 475 -0.144 – – –
Almeida et al. 2025 1.38 2.25 – 70 – 1698 – –
Zhang et al. 2024 – – – – -0.073* – – –
Hunt & Reffert 2024 – – – – – 2290* – –
Cavallo et al. 2024 1.64 2.23 – 263 0.470 – – –
Hunt & Reffert 2023 1.38 2.06 1.62 247 – – – –
Almeida et al. 2023 1.35 2.23 – 170 -0.004 850* 0.51 –
Just et al. 2023 – – – 316 – 42 – –
Tarricq et al. 2022 1.48 – – 363 – – – –
Jaehnig et al. 2021 1.46* – – – – – – –
Rain et al. 2021 1.47 2.08 – 129 – – – 0
Dias et al. 2021 1.38 2.25 – 70 0.034 – – –
Cantat-Gaudin et al. 2020 1.55 1.60 – 288 – – – –
Cantat-Gaudin & Anders 2020 1.47 – – – – – – –
Liu & Pang 2019 – – – 355 -0.500 – – –
Soubiran et al. 2018 1.47 – – – – – – –
Cantat-Gaudin et al. 2018 1.47 – – – – – – –
Loktin & Popova 2017 1.05 2.00 – 195 – – – –
Kharchenko et al. 2016 1.40 2.08 – 316 – – – –
Kharchenko et al. 2013 1.40 2.08 – 316 – – – –
Gozha et al. 2012 1.32 – – 129 – – – –
Kharchenko et al. 2012 1.40 2.08 – 316 – – – –
van den Bergh 2006 1.32 2.08 – 129 – – – –
Dias et al. 2002 1.32 2.08 – 129 – – – –

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

Visualization

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