Collinder 313
(VDBH 198; NGC 6208; MWSC 2470; OCL 964; vdBergh-Hagen 198; ESO 179 14; FSR 1724; FoF 2063)
Summary
Collinder 313 is a rich, very dense object of very high C3 quality. It is located at a relatively close 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) | 252.367 | -53.728 | – | -0.24 | 0.53 | -32.47 |
| Chen et al. (2003) | 252.355 | -53.729 | – | – | – | – |
| Kharchenko et al. (2005) | 252.36 | -53.73 | – | -0.91 | -4.72 | – |
| Kharchenko et al. (2007) | 252.36 | -53.73 | – | 0.14 | – | – |
| Piskunov et al. (2008) | 252.356 | -53.729 | – | – | – | – |
| Kharchenko et al. (2013) | 252.345 | -53.715 | – | -3.15 | -2.2 | -32.2 |
| Kharchenko et al. (2016) | 252.333 | -53.715 | – | – | – | – |
| Loktin & Popova (2017) | 252.36 | -53.729 | – | 1.653 | 0.238 | -32.2 |
| Cantat-Gaudin et al. (2018) | 252.336 | -53.714 | 0.83 | -0.966 | -1.519 | – |
| Bica et al. (2019) | 252.355 | -53.729 | – | – | – | – |
| Soubiran et al. (2018) | 252.336 | -53.714 | – | – | – | -32.15 |
| Bossini et al. (2019) | 252.336 | -53.714 | – | – | – | – |
| Liu & Pang (2019) | 252.343 | -53.725 | 0.842 | -0.952 | -1.506 | – |
| Cantat-Gaudin et al. (2020) | 252.336 | -53.714 | 0.83 | -0.966 | -1.519 | – |
| Dias et al. (2021) | 252.327 | -53.713 | 0.832 | -0.974 | -1.502 | -31.761 |
| Tarricq et al. (2022) | 252.351 | -53.717 | 0.838 | -0.994 | -1.527 | – |
| He et al. (2022) | 252.335 | -53.727 | 0.849 | -1.006 | -1.528 | – |
| Just et al. (2023) | 252.333 | -53.715 | – | – | – | – |
| Cordoni et al. (2023) | 252.327 | -53.713 | 0.832 | -0.974 | -1.502 | – |
| Hunt & Reffert (2023) | 252.344 | -53.712 | 0.846 | -1.015 | -1.521 | -32.727 |
| Cavallo et al. (2024) | 252.334 | -53.72 | 0.847 | – | – | – |
| Hunt & Reffert (2024) | 252.344 | -53.712 | 0.846 | -1.015 | -1.521 | -32.727 |
| Almeida et al. (2025) | 252.327 | -53.713 | – | – | – | – |
| Hu & Soubiran (2025) | 252.334 | -53.72 | – | – | – | – |
| UCC | 252.338 | -53.721 | 0.844 | -1.001 | -1.523 | -32.461 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.21, Dist=939.0, Age=9.069, [Fe/H]=-0.03 |
| Chen et al. (2003) | E(B-V)=0.21, HDis=939, Age=1.17, [Fe/H]_1=-0.03 |
| Kharchenko et al. (2005) | E(B-V)=0.21, Dist=939, logt=9.07 |
| Piskunov et al. (2008) | E(B-V)=0.21, Dist=939, logt=9.07, logMA=1.149 |
| Kharchenko et al. (2013) | E(B-V)=0.208, d=926.0, logt=9.28, [Fe/H]=-0.03 |
| Kharchenko et al. (2016) | E(B-V)=0.208, d=926.0, logt=9.28 |
| Loktin & Popova (2017) | E(B-V)=0.209, Dist=956, logt=9.073 |
| Cantat-Gaudin et al. (2018) | dmode=1164.4 |
| Soubiran et al. (2018) | dmode=1164.4 |
| Bossini et al. (2019) | AV=0.631, Dist=10.345, logA=9.223, Fe/H=-0.01 |
| Liu & Pang (2019) | Age=1.51, Z=0.0 |
| Cantat-Gaudin et al. (2020) | AVNN=0.66, DistPc=1215.0, AgeNN=9.15 |
| Dias et al. (2021) | Av=0.91, Dist=1143, logage=9.282, [Fe/H]=-0.089 |
| Tarricq et al. (2022) | Dist=1182, logAgeNN=9.17 |
| He et al. (2022) | A0=0.8, logAge=9.25 |
| Just et al. (2023) | logt=9.28, logmt=1.926 |
| Cordoni et al. (2023) | Av=0.91, Dist=10.29, logAge=9.282, [Fe/H]=-0.089, mass-single=384.649, fbin-tot=0.646, fbss-MS=0.017 |
| Hunt & Reffert (2023) | AV50=0.529, diffAV50=0.216, MOD50=10.244, logAge50=9.212 |
| Cavallo et al. (2024) | AV50=0.88, dMod50=10.37, logAge50=9.16, [Fe/H]50=0.16 |
| Hunt & Reffert (2024) | MassJ=1169.39, MassTot=1195.77 |
| Almeida et al. (2025) | AV=0.91, Dist=1143, logAge=9.282, MassRk=937.6 |
| Hu & Soubiran (2025) | MA22=-0.19, MA23f=-0.23, MA23g=-0.22, MZ23=-0.31, MK24=-0.2, MF24=-0.24 |
Search coordinates in Bayestar19