NGC 1513
(MWSC 346; FoF 184)
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
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
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | β | 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 | β |
| Almeida et al. | 2025 | 62.475 | 49.507 | β | β | β | β |
| Zhang et al. | 2024 | 62.472 | 49.502 | β | β | β | β |
| 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 | β | β | β |
| Hunt & Reffert | 2023 | 62.472 | 49.502 | 0.677 | 1.296 | -3.693 | -14.938 |
| Almeida et al. | 2023 | 62.458 | 49.503 | β | β | β | β |
| Just et al. | 2023 | 62.414 | 49.509 | β | β | β | β |
| Tarricq et al. | 2022 | 62.476 | 49.494 | 0.673 | 1.318 | -3.699 | β |
| Jaehnig et al. | 2021 | 62.465 | 49.503 | 0.686 | 1.3 | -3.67 | β |
| Rain et al. | 2021 | 62.47 | 49.504 | 0.651 | 1.324 | -3.679 | β |
| 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 | β |
| SΓ‘nchez et al. | 2020 | 62.487 | 49.515 | β | 1.487 | -3.483 | β |
| Cantat-Gaudin & Anders | 2020 | 62.47 | 49.504 | 0.651 | 1.324 | -3.679 | β |
| Liu & Pang | 2019 | 62.485 | 49.498 | 0.644 | 1.327 | -3.677 | β |
| Soubiran et al. | 2018 | 62.47 | 49.504 | β | β | β | -14.73 |
| Cantat-Gaudin et al. | 2018 | 62.47 | 49.504 | 0.651 | 1.324 | -3.679 | β |
| Loktin & Popova | 2017 | 62.49 | 49.516 | β | -1.084 | -5.576 | -15.1 |
| Kharchenko et al. | 2016 | 62.414 | 49.509 | β | β | β | β |
| Dias et al. | 2014 | 62.487 | 49.515 | β | 1.11 | -4.66 | β |
| Kharchenko et al. | 2013 | 62.425 | 49.51 | β | -1.08 | -3.49 | -15.1 |
| Gozha et al. | 2012 | 62.488 | 49.515 | β | β | β | β |
| Kharchenko et al. | 2012 | 62.425 | 49.51 | β | -1.08 | -3.49 | -15.13 |
| van den Bergh | 2006 | 62.65 | 49.517 | β | β | β | β |
| Dias et al. | 2002 | 62.487 | 49.515 | β | 1.11 | -4.66 | -15.13 |
π‘ 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 | β | 475 | -0.144 | β | β | β |
| Almeida et al. | 2025 | 1.38 | 2.25 | β | 70 | β | 1698 | β | β |
| Zhang et al. | 2024 | β | β | β | β | -0.073* | β | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 2290* | β | β |
| Cavallo et al. | 2024 | 1.64 | 2.23 | β | 263 | 0.470 | β | β | β |
| Hunt & Reffert | 2023 | 1.38 | 2.06 | 1.62 | 247 | β | β | β | β |
| Almeida et al. | 2023 | 1.35 | 2.23 | β | 170 | -0.004 | 850* | 0.51 | β |
| Just et al. | 2023 | β | β | β | 316 | β | 42 | β | β |
| Tarricq et al. | 2022 | 1.48 | β | β | 363 | β | β | β | β |
| Jaehnig et al. | 2021 | 1.46* | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 1.47 | 2.08 | β | 129 | β | β | β | 0 |
| Dias et al. | 2021 | 1.38 | 2.25 | β | 70 | 0.034 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 1.55 | 1.60 | β | 288 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 1.47 | β | β | β | β | β | β | β |
| Liu & Pang | 2019 | β | β | β | 355 | -0.500 | β | β | β |
| Soubiran et al. | 2018 | 1.47 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 1.47 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 1.05 | 2.00 | β | 195 | β | β | β | β |
| Kharchenko et al. | 2016 | 1.40 | 2.08 | β | 316 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.40 | 2.08 | β | 316 | β | β | β | β |
| Gozha et al. | 2012 | 1.32 | β | β | 129 | β | β | β | β |
| Kharchenko et al. | 2012 | 1.40 | 2.08 | β | 316 | β | β | β | β |
| van den Bergh | 2006 | 1.32 | 2.08 | β | 129 | β | β | β | β |
| Dias et al. | 2002 | 1.32 | 2.08 | β | 129 | β | β | β | β |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.