Ruprecht 67
(MWSC 1534; OCL 748; ESO 260 01)
Summary
Ruprecht 67 is a rich, very dense object of high C3 quality. It is located at a relatively close distance from the Sun, near the mid-plane. It is very well-studied in the literature.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 130.412 | -43.367 | – | -2.66 | 2.56 | -15.4 |
| Kharchenko et al. (2003) | 130.41 | -43.37 | – | -9.85 | 1.92 | – |
| Kharchenko et al. (2005) | 130.41 | -43.37 | – | -9.95 | 2.23 | – |
| Kharchenko et al. (2007) | 130.41 | -43.37 | – | 0.12 | – | – |
| Piskunov et al. (2008) | 130.398 | -43.366 | – | – | – | – |
| Kharchenko et al. (2013) | 130.44 | -43.395 | – | -10.05 | 3.2 | -15.4 |
| Kharchenko et al. (2016) | 130.435 | -43.392 | – | – | – | – |
| Loktin & Popova (2017) | 130.44 | -43.395 | – | -7.349 | 5.376 | -15.4 |
| Cantat-Gaudin et al. (2018) | 130.464 | -43.363 | 0.624 | -4.42 | 3.646 | – |
| Bica et al. (2019) | 130.458 | -43.357 | – | – | – | – |
| Bossini et al. (2019) | 130.464 | -43.363 | – | – | – | – |
| Cantat-Gaudin et al. (2020) | 130.464 | -43.363 | 0.624 | -4.42 | 3.646 | – |
| Dias et al. (2021) | 130.455 | -43.361 | 0.623 | -4.445 | 3.644 | – |
| Rain et al. (2021) | 130.464 | -43.363 | 0.624 | -4.42 | 3.646 | – |
| Jaehnig et al. (2021) | 130.463 | -43.364 | 0.652 | -4.373 | 3.685 | – |
| Just et al. (2023) | 130.435 | -43.392 | – | – | – | – |
| Hunt & Reffert (2023) | 130.473 | -43.368 | 0.626 | -4.329 | 3.707 | 16.895 |
| Cavallo et al. (2024) | 130.476 | -43.353 | 0.626 | – | – | – |
| Hunt & Reffert (2024) | 130.473 | -43.368 | 0.626 | -4.329 | 3.707 | 16.895 |
| Almeida et al. (2025) | 130.455 | -43.361 | – | – | – | – |
| Hu & Soubiran (2025) | 130.476 | -43.353 | – | – | – | – |
| UCC | 130.477 | -43.363 | 0.628 | -4.371 | 3.69 | 9.377 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.432, Dist=1504.0, Age=8.256 |
| Kharchenko et al. (2003) | E(B-V)=0.43, Dist=1515 |
| Kharchenko et al. (2005) | E(B-V)=0.43, Dist=1504, logt=8.38 |
| Piskunov et al. (2008) | E(B-V)=0.43, Dist=1504, logt=8.38, logMA=2.192 |
| Kharchenko et al. (2013) | E(B-V)=0.5, d=1342.0, logt=8.6 |
| Kharchenko et al. (2016) | E(B-V)=0.5, d=1342.0, logt=8.6 |
| Loktin & Popova (2017) | E(B-V)=0.429, Dist=1546, logt=8.282 |
| Cantat-Gaudin et al. (2018) | dmode=1532.3 |
| Bossini et al. (2019) | AV=1.292, Dist=11.08, logA=8.651, Fe/H=0.0 |
| Cantat-Gaudin et al. (2020) | AVNN=1.26, DistPc=1607.0, AgeNN=8.63 |
| Dias et al. (2021) | Av=1.795, Dist=1459, logage=7.845, [Fe/H]=0.008 |
| Rain et al. (2021) | E(B-V)=0.43, Dist=1532.3, log(Age)=8.25, NBSS=0 |
| Jaehnig et al. (2021) | dmode=1.534 |
| Just et al. (2023) | logt=8.6, logmt=2.075 |
| Hunt & Reffert (2023) | AV50=1.655, diffAV50=2.233, MOD50=10.893, logAge50=8.067 |
| Cavallo et al. (2024) | AV50=1.37, dMod50=10.75, logAge50=8.71, [Fe/H]50=0.3 |
| Hunt & Reffert (2024) | MassJ=350.910, MassTot=357.763 |
| Almeida et al. (2025) | AV=1.795, Dist=1459, logAge=7.845, MassRk=232.8 |
| Hu & Soubiran (2025) | MA22=-0.21, MA23f=-0.22, MZ23=-0.11, MK24=-0.16, MF24=-0.18 |
Search coordinates in Bayestar19