NGC 744
(Collinder 22; MWSC 153; FSR 0574; FoF 669)
0.91
UTI
0.81
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Nm (P>50%)
261
Core radius and density
1.5 [pc], 9.8 [pc-2]
- CN 0.81 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
NGC 744 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is very well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999β | 29.651 | 55.471 | 0.733 | -1.865 | -1.871 | -25.861 |
| Li et al. | 2025 | 29.652 | 55.473 | 0.729 | -1.864 | -1.79 | β |
| Yang et al. | 2025 | 29.642 | 55.481 | β | β | β | β |
| Almeida et al. | 2025 | 29.66 | 55.475 | β | β | β | β |
| Zhang et al. | 2024 | 29.642 | 55.481 | β | β | β | β |
| Hunt & Reffert | 2024 | 29.642 | 55.481 | 0.721 | -1.869 | -1.883 | -27.237 |
| Cavallo et al. | 2024 | 29.638 | 55.474 | 0.724 | β | β | β |
| Hunt & Reffert | 2023 | 29.642 | 55.481 | 0.721 | -1.869 | -1.883 | -27.237 |
| Almeida et al. | 2023 | 29.655 | 55.48 | β | β | β | β |
| Just et al. | 2023 | 29.634 | 55.475 | β | β | β | β |
| Tarricq et al. | 2022 | 29.645 | 55.459 | 0.714 | -1.837 | -1.885 | β |
| Jaehnig et al. | 2021 | 29.663 | 55.471 | 0.761 | -1.876 | -1.737 | β |
| Rain et al. | 2021 | 29.652 | 55.473 | 0.729 | -1.864 | -1.79 | β |
| Richer et al. | 2021 | 29.663 | 55.469 | 0.73 | -1.871 | -1.738 | β |
| Dias et al. | 2021 | 29.66 | 55.475 | 0.732 | -1.885 | -1.804 | β |
| Cantat-Gaudin et al. | 2020 | 29.652 | 55.473 | 0.729 | -1.864 | -1.79 | β |
| SΓ‘nchez et al. | 2020 | 29.637 | 55.473 | β | -1.735 | -1.431 | β |
| Zhong et al. | 2020 | 29.652 | 55.473 | β | -1.864 | -1.79 | -39.11 |
| Cantat-Gaudin & Anders | 2020 | 29.652 | 55.473 | 0.729 | -1.864 | -1.79 | β |
| Liu & Pang | 2019 | 29.656 | 55.485 | 0.729 | -1.872 | -1.763 | β |
| Soubiran et al. | 2018 | 29.652 | 55.473 | β | β | β | -25.47 |
| Bica et al. | 2019 | 29.669 | 55.478 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 29.652 | 55.473 | 0.729 | -1.864 | -1.79 | β |
| Dias et al. | 2018 | β | β | β | -1.66 | -1.67 | β |
| Dib et al. | 2018 | 29.644 | 55.478 | β | β | β | β |
| Loktin & Popova | 2017 | 29.64 | 55.473 | β | 0.021 | -1.35 | β |
| Sampedro et al. | 2017 | 29.637 | 55.473 | β | -2.69 | -2.36 | β |
| Joshi et al. | 2016 | 29.644 | 55.478 | β | β | β | β |
| Kharchenko et al. | 2016 | 29.634 | 55.475 | β | β | β | β |
| Dias et al. | 2014 | 29.637 | 55.473 | β | -2.97 | -2.01 | β |
| Kharchenko et al. | 2013 | 29.644 | 55.478 | β | -0.3 | -3.92 | β |
| Kharchenko et al. | 2012 | 29.644 | 55.478 | β | -0.81 | -4.01 | β |
| Bukowiecki et al. | 2011 | 29.7 | 55.462 | β | β | β | β |
| Piskunov et al. | 2008 | 29.626 | 55.464 | β | β | β | β |
| Piskunov et al. | 2007 | 29.626 | 55.464 | β | β | β | β |
| Ahumada & Lapasset | 2007 | 29.625 | 55.467 | β | β | β | β |
| van den Bergh | 2006 | 29.65 | 55.467 | β | β | β | β |
| Kharchenko et al. | 2005 | 29.64 | 55.47 | β | -2.85 | -3.15 | β |
| Kharchenko et al. | 2003 | 29.65 | 55.47 | β | -1.8 | -3.81 | β |
| Dias et al. | 2002 | 29.637 | 55.473 | β | -1.34 | 1.15 | β |
| Dambis | 1999 | 29.65 | 55.467 | β | β | β | β |
| Lynga | 1987 | 29.614 | 55.476 | β | β | β | β |
| Sulentic et al. | 1973 | 29.645 | 55.471 | β | β | β | β |
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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999β | 1.32 | 1.2 | 1.81 | 237 | -0.154 | 280 | 0.53 | 0 |
| Li et al. | 2025 | 1.17 | 0.85 | β | 646 | -0.247 | β | β | β |
| Yang et al. | 2025 | β | β | β | 347 | -0.210(3) | β | β | β |
| Almeida et al. | 2025 | 1.26 | 1.12 | β | 182 | β | 244 | β | β |
| Zhang et al. | 2024 | β | β | β | β | -0.142(1) | β | β | β |
| Hunt & Reffert | 2024 | 1.30 | 0.91 | 1.81 | 344 | β | 832(1) | β | β |
| Cavallo et al. | 2024 | 1.44 | 1.22 | β | 257 | 0.180 | β | β | β |
| Hunt & Reffert | 2023 | 1.30 | 0.91 | 1.81 | 344 | β | β | β | β |
| Almeida et al. | 2023 | 1.26 | 1.27 | β | 220 | -0.046 | 315(1) | 0.53 | β |
| Just et al. | 2023 | β | β | β | 237 | β | 601 | β | β |
| Tarricq et al. | 2022 | 1.33 | β | β | 162 | β | β | β | β |
| Jaehnig et al. | 2021 | 1.31(1) | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 1.32 | 1.20 | β | 174 | β | β | β | 0 |
| Richer et al. | 2021 | β | 0.99 | β | β | β | β | β | β |
| Dias et al. | 2021 | 1.26 | 1.12 | β | 182 | 0.019 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 1.37 | 0.84 | β | 135 | β | β | β | β |
| Kounkel et al. | 2020 | 1.33 | 1.14 | β | 347 | β | β | β | β |
| Zhong et al. | 2020 | 1.32(1) | 1.20 | β | 8375 | -0.166 | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 1.32 | β | β | β | β | β | β | β |
| Liu & Pang | 2019 | β | β | β | 479 | -0.500 | β | β | β |
| Soubiran et al. | 2018 | 1.32 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 1.32 | β | β | β | β | β | β | β |
| Dib et al. | 2018 | 1.38 | β | β | 237 | β | β | β | β |
| Loktin & Popova | 2017 | 1.25 | 1.20 | β | 176 | β | β | β | β |
| Joshi et al. | 2016 | 1.38 | 1.20 | β | 237 | β | 219 | β | β |
| Kharchenko et al. | 2016 | 1.38 | 1.20 | β | 237 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.38 | 1.20 | β | 237 | β | β | β | β |
| Bukowiecki et al. | 2012 | β | β | β | β | β | 424 | β | β |
| Kharchenko et al. | 2012 | 1.38 | 1.20 | β | 237 | β | β | β | β |
| Bukowiecki et al. | 2011 | 1.45(1) | 1.23 | β | 112 | β | β | β | β |
| Piskunov et al. | 2008 | 1.21 | 1.20 | β | 257 | β | 56(1) | β | β |
| Piskunov et al. | 2007 | 1.21 | 1.20 | β | 257 | β | 15 | β | β |
| Ahumada & Lapasset | 2007 | β | 1.20 | β | 178 | β | β | β | 1 |
| van den Bergh | 2006 | 1.21 | 1.20 | β | 178 | β | β | β | β |
| Kharchenko et al. | 2005 | 1.21 | 1.20 | β | 257 | β | β | β | β |
| Kharchenko et al. | 2003 | 1.20 | 1.20 | β | β | β | β | β | β |
| Dias et al. | 2002 | 1.21 | 1.21 | β | 177 | β | β | β | β |
| Dambis | 1999 | 1.04 | 1.58 | β | 126 | β | β | β | β |
| Lynga | 1987 | 1.50 | 1.20 | β | 39 | β | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Palma et al. (2025)
Classified as optical pair P555, along with Stock_4.
Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit. Silver sample.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.99 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.99 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.1517, e_all=0.0975.
Ahumada & Lapasset (2007)
Star 7 has a spectrum A05 (1965ApJS...12..215H).