Hogg 4
(MWSC 1734; OCL 793; ESO 167 13; FSR 1515)
0.94
UTI
1.0
CN
1.0
Cdens
1.0
CC3
0.86
Clit
1.0
Cdup
Radius (P>50% members)
5.2 [arcmin]
- CN 1.0 Very rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.86 Well-studied
- Cdup 1.0 Unique
Overview
Hogg 4 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a moderate 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 and mass parameters (see Parameters). It is well-studied in the literature.
Distant
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 | 149.415 | -54.616 | 0.238 | -5.034 | 4.476 | 26.492 |
| Li et al. | 2025 | 149.424 | -54.612 | 0.21 | -5.022 | 4.484 | β |
| Hu & Soubiran | 2025 | 149.404 | -54.61 | β | β | β | β |
| Almeida et al. | 2025 | 149.423 | -54.608 | β | β | β | β |
| Hunt & Reffert | 2024 | 149.427 | -54.632 | 0.243 | -5.035 | 4.472 | 23.941 |
| Cavallo et al. | 2024 | 149.404 | -54.61 | 0.241 | β | β | β |
| Hunt & Reffert | 2023 | 149.427 | -54.632 | 0.243 | -5.035 | 4.472 | 23.941 |
| Almeida et al. | 2023 | 149.414 | -54.61 | β | β | β | β |
| Just et al. | 2023 | 149.462 | -54.622 | β | β | β | β |
| Dias et al. | 2021 | 149.423 | -54.608 | 0.205 | -5.016 | 4.503 | 26.578 |
| Cantat-Gaudin et al. | 2020 | 149.424 | -54.612 | 0.21 | -5.022 | 4.484 | β |
| Cantat-Gaudin & Anders | 2020 | 149.424 | -54.612 | 0.21 | -5.022 | 4.484 | β |
| Soubiran et al. | 2018 | 149.424 | -54.612 | β | β | β | 26.57 |
| Bica et al. | 2019 | 149.435 | -54.622 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 149.424 | -54.612 | 0.21 | -5.022 | 4.484 | β |
| Kharchenko et al. | 2016 | 149.462 | -54.622 | β | β | β | β |
| Kharchenko et al. | 2013 | 149.467 | -54.625 | β | -1.9 | 1.5 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 3.60 | 1.83 | β | 1076 | 0.045 | β | β | β |
| Hu & Soubiran | 2025 | β | β | β | β | -0.150* | β | β | β |
| Almeida et al. | 2025 | 3.71 | 1.93 | β | 982 | β | 1943 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 5453* | β | β |
| Cavallo et al. | 2024 | 3.01 | 1.82 | β | 1230 | 0.110 | β | β | β |
| Hunt & Reffert | 2023 | 3.72 | 1.84 | 1.70 | 822 | β | β | β | β |
| Almeida et al. | 2023 | 3.48 | 1.92 | β | 998 | -0.046 | 2165* | 0.73 | β |
| Just et al. | 2023 | β | β | β | 200 | β | 70 | β | β |
| Dias et al. | 2021 | 3.71 | 1.93 | β | 982 | -0.044 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 4.02 | 1.04 | β | 1479 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 4.18 | β | β | β | β | β | β | β |
| Soubiran et al. | 2018 | 4.18 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 4.18 | β | β | β | β | β | β | β |
| Kharchenko et al. | 2016 | 1.77 | 1.03 | β | 200 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.77 | 1.03 | β | 200 | β | β | β | β |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit. Silver sample.
Cavallo et al. (2024)
Gold sample.
Dias et al. (2002)
No cluster (Piatti, A. E.; ClariΓ‘, J. J.; Ahumada, A. V. 2011, NewA 16, 161)