Andrews Lindsay 5
(MWSC 2985)
0.88
UTI
0.82
CN
1.0
Cdens
1.0
CC3
0.78
Clit
1.0
Cdup
Stellar density (N50/rad)
57.8 [N/pc2]
- CN 0.82 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.78 Well-studied
- Cdup 1.0 Unique
Overview
Andrews Lindsay 5 is a rich, very dense object of very high C3 quality. Its parallax locates it at a large* distance, near the mid-plane, affected by very high extinction. It is catalogued as a massive, metal-poor, very young cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is well-studied in the literature.
(*): The parallax distance estimate (~5.49 kpc) differs significantly from the median photometric distance (~3.42 kpc).
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999β | 281.078 | -4.928 | 0.182 | -0.88 | -3.621 | 67.635 |
| Hunt & Reffert | 2024 | 281.078 | -4.93 | 0.213 | -0.916 | -3.656 | 71.902 |
| Celli et al. | 2024 | 281.079 | -4.931 | β | β | β | β |
| Cavallo et al. | 2024 | 281.08 | -4.931 | 0.209 | β | β | β |
| Hunt & Reffert | 2023 | 281.078 | -4.93 | 0.213 | -0.916 | -3.656 | 71.902 |
| Just et al. | 2023 | 281.077 | -4.932 | β | β | β | β |
| Cantat-Gaudin et al. | 2020 | 281.079 | -4.931 | 0.137 | -0.901 | -3.562 | β |
| SΓ‘nchez et al. | 2020 | 281.079 | -4.93 | β | -1.066 | -3.793 | β |
| Cantat-Gaudin & Anders | 2020 | 281.079 | -4.931 | 0.137 | -0.901 | -3.562 | β |
| Soubiran et al. | 2018 | 281.079 | -4.931 | β | β | β | 59.08 |
| Cantat-Gaudin et al. | 2018 | 281.079 | -4.931 | 0.137 | -0.901 | -3.562 | β |
| Kharchenko et al. | 2016 | 281.077 | -4.932 | β | β | β | β |
| Dias et al. | 2014 | 281.079 | -4.93 | β | 1.02 | -1.66 | β |
| Kharchenko et al. | 2013 | 281.085 | -4.93 | β | 2.59 | -6.33 | β |
| Dias et al. | 2002 | 281.079 | -4.93 | β | 2.59 | -6.33 | 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 | 3.42 | 7.49 | 2.74 | 1 | -0.820 | 1030 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 4240(1) | β | β |
| Celli et al. | 2024 | β | β | β | 1 | β | 1030 | β | β |
| Cavallo et al. | 2024 | 2.78 | 5.11 | β | 120 | -0.820 | β | β | β |
| Hunt & Reffert | 2023 | 4.06 | 4.42 | 2.74 | 108 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 1 | β | 433 | β | β |
| Cantat-Gaudin & Anders | 2020 | 6.01 | β | β | β | β | β | β | β |
| Soubiran et al. | 2018 | 6.01 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 6.01 | β | β | β | β | β | β | β |
| Kharchenko et al. | 2016 | 2.29 | 7.49 | β | 1 | β | β | β | β |
| Kharchenko et al. | 2013 | 2.29 | 7.49 | β | 1 | β | β | β | β |
| Dias et al. | 2002 | 2.29 | 7.49 | β | 1 | β | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Silver sample.