ESO 368 11
(FSR 1353; MWSC 1320; MWSC 1321; FoF 38)
Summary
ESO 368 11 is a rich, very dense object of very high C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It is very well-studied in the literature.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 116.092 | -34.619 | – | -0.59 | 3.25 | – |
| Froebrich et al. (2007) | 116.104 | -34.632 | – | – | – | – |
| Glushkova et al. (2010) | 116.093 | -34.619 | – | – | – | – |
| Kharchenko et al. (2013) | 116.1 | -34.627 | – | -5.59 | 6.96 | – |
| Kharchenko et al. (2016) | 116.094 | -34.624 | – | – | – | – |
| Loktin & Popova (2017) | 116.07 | -34.619 | – | -4.704 | 6.497 | – |
| Cantat-Gaudin et al. (2018) | 116.086 | -34.628 | 0.429 | -0.853 | 2.278 | – |
| Bica et al. (2019) | 116.096 | -34.636 | – | – | – | – |
| Soubiran et al. (2018) | 116.086 | -34.628 | – | – | – | 22.47 |
| Bossini et al. (2019) | 116.086 | -34.628 | – | – | – | – |
| Liu & Pang (2019) | 116.093 | -34.633 | 0.433 | -0.86 | 2.258 | – |
| Cantat-Gaudin et al. (2020) | 116.086 | -34.628 | 0.429 | -0.853 | 2.278 | – |
| Dias et al. (2021) | 116.092 | -34.633 | 0.432 | -0.858 | 2.237 | – |
| Just et al. (2023) | 116.094 | -34.624 | – | – | – | – |
| Hunt & Reffert (2023) | 116.083 | -34.63 | 0.448 | -0.834 | 2.301 | 21.733 |
| Cavallo et al. (2024) | 116.087 | -34.63 | 0.451 | – | – | – |
| Hunt & Reffert (2024) | 116.083 | -34.63 | 0.448 | -0.834 | 2.301 | 21.733 |
| Almeida et al. (2025) | 116.092 | -34.633 | – | – | – | – |
| UCC | 116.086 | -34.625 | 0.448 | -0.833 | 2.295 | 21.717 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.06, Dist=1490.0, Age=9.0 |
| Glushkova et al. (2010) | E(B-V)=0.06, Dist=1490.0, Age=9.0 |
| Kharchenko et al. (2013) | E(B-V)=0.073, d=1245.0, logt=8.945 |
| Kharchenko et al. (2016) | E(B-V)=0.073, d=1245.0, logt=8.945 |
| Loktin & Popova (2017) | E(B-V)=0.67, Dist=3862, logt=7.89 |
| Cantat-Gaudin et al. (2018) | dmode=2181.7 |
| Soubiran et al. (2018) | dmode=2181.7 |
| Bossini et al. (2019) | AV=0.818, Dist=11.168, logA=9.011, Fe/H=0.0 |
| Liu & Pang (2019) | Age=0.355, Z=0.25 |
| Cantat-Gaudin et al. (2020) | AVNN=1.11, DistPc=2117.0, AgeNN=8.77 |
| Dias et al. (2021) | Av=1.737, Dist=1899, logage=8.571, [Fe/H]=0.016 |
| Just et al. (2023) | logt=8.945, logmt=1.955 |
| Hunt & Reffert (2023) | AV50=1.572, diffAV50=1.082, MOD50=11.553, logAge50=8.526 |
| Cavallo et al. (2024) | AV50=1.79, dMod50=11.92, logAge50=8.51, [Fe/H]50=0.5 |
| Hunt & Reffert (2024) | MassJ=701.610, MassTot=701.610 |
| Almeida et al. (2025) | AV=1.737, Dist=1899, logAge=8.571, MassRk=547.3 |
Search coordinates in Bayestar19