Collinder 135
(FoF 2386; OCSN 190)
Summary
Collinder 135 is a rich, very dense object of very high C3 quality. It is located at a very close distance from the Sun, near the mid-plane. It is very well-studied in the literature.
This object shares a very small percentage of members with 3 later reported entries.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 109.321 | -36.817 | – | -10.7 | 5.3 | 15.85 |
| Chen et al. (2003) | 109.263 | -36.877 | – | -10.55 | 6.27 | 34.0 |
| Piskunov et al. (2007) | 109.445 | -37.156 | – | – | – | – |
| Piskunov et al. (2008) | 109.445 | -37.156 | – | – | – | – |
| Kharchenko et al. (2012) | 109.485 | -37.035 | – | -9.33 | 5.26 | – |
| Loktin & Popova (2017) | 109.32 | -36.817 | – | -10.7 | 5.3 | 15.4 |
| Cantat-Gaudin et al. (2018) | 109.362 | -37.044 | 3.278 | -9.975 | 6.157 | – |
| Soubiran et al. (2018) | 109.362 | -37.044 | – | – | – | 16.03 |
| Dias et al. (2019) | 109.362 | -37.044 | 3.278 | -9.975 | 6.157 | 16.719 |
| Liu & Pang (2019) | 109.594 | -37.01 | 3.301 | -10.107 | 6.192 | – |
| Cantat-Gaudin et al. (2020) | 109.362 | -37.044 | 3.278 | -9.975 | 6.157 | – |
| Dias et al. (2021) | 109.233 | -37.099 | 3.286 | -9.977 | 6.211 | 16.513 |
| Rain et al. (2021) | 109.362 | -37.044 | 3.278 | -9.975 | 6.157 | – |
| Jaehnig et al. (2021) | 109.459 | -37.008 | 3.355 | -10.18 | 6.279 | – |
| He et al. (2022) | 109.363 | -36.869 | 3.333 | -10.116 | 6.143 | – |
| Qin et al. (2023) | 109.52 | -36.88 | 3.35 | -10.07 | 6.24 | 15.0 |
| Hunt & Reffert (2023) | 109.406 | -36.921 | 3.331 | -10.078 | 6.23 | 13.166 |
| Cavallo et al. (2024) | 109.412 | -36.904 | 3.333 | – | – | – |
| Celli et al. (2024) | 109.362 | -37.044 | – | – | – | – |
| Hunt & Reffert (2024) | 109.406 | -36.921 | 3.331 | -10.078 | 6.23 | 13.166 |
| Alfonso et al. (2024) | 109.433 | -36.948 | 3.319 | -10.116 | 6.242 | – |
| Almeida et al. (2025) | 109.233 | -37.099 | – | – | – | – |
| UCC | 109.363 | -36.948 | 3.34 | -10.036 | 6.221 | 15.099 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.032, Dist=316.0, Age=7.407, [Fe/H]=-0.219 |
| Chen et al. (2003) | HDis=316, Age=0.02 |
| Piskunov et al. (2007) | E(B-V)=0.04, Dist=319, logt=7.54, logM=2.537 |
| Piskunov et al. (2008) | E(B-V)=0.04, Dist=319, logt=7.54, logM=2.76, logMA=2.736 |
| Kharchenko et al. (2012) | e_bv=0.042, distance=361, log_age=7.6, metallicity=-0.219 |
| Loktin & Popova (2017) | E(B-V)=0.035, Dist=316, logt=7.407 |
| Cantat-Gaudin et al. (2018) | dmode=302.4 |
| Soubiran et al. (2018) | dmode=302.4 |
| Dias et al. (2019) | E(B-V)=0.07, Dist=310, logAge=7.575, Z=0.018 |
| Liu & Pang (2019) | Age=0.055, Z=0.5 |
| Cantat-Gaudin et al. (2020) | AVNN=0.01, DistPc=292.0, AgeNN=7.42 |
| Dias et al. (2021) | Av=0.18, Dist=307, logage=7.669, [Fe/H]=0.111 |
| Rain et al. (2021) | E(B-V)=0.03, Dist=302.4, log(Age)=7.4, NBSS=0 |
| Jaehnig et al. (2021) | dmode=0.299 |
| He et al. (2022) | A0=0.35, logAge=7.55 |
| Qin et al. (2023) | E(B-V)=0.1, m-M=7.64, logt=7.65 |
| Hunt & Reffert (2023) | AV50=0.107, diffAV50=0.567, MOD50=7.338, logAge50=7.475 |
| Cavallo et al. (2024) | AV50=0.57, dMod50=7.41, logAge50=7.42, [Fe/H]50=0.14 |
| Celli et al. (2024) | Age=26.3, Mc=305.4 |
| Hunt & Reffert (2024) | MassJ=119.509, MassTot=128.298 |
| Alfonso et al. (2024) | AV=0.01041, MOD=7.32994, logAge=7.60422, Z=0.11142 |
| Almeida et al. (2025) | AV=0.18, Dist=307, logAge=7.669, MassRk=311.8 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Alessi 36 | 2.4 | 106.61 | -37.64 | 3.61 | -9.66 | 7.08 | 15.36 | 0.32 |
| OCSN 210 | 2.4 | 106.61 | -37.67 | 3.6 | -9.68 | 7.09 | 15.36 | 0.01 |
| UBC 7 | 0.7 | 106.63 | -37.7 | 3.59 | -9.69 | 7.06 | 15.28 | 0.7 |