Teutsch 35
(ASCC 103; MWSC 3141; Teutsch J1935.9+3540; FoF 2426; OCSN 275)
Summary
Teutsch 35 is a rich, very dense object of very high C3 quality. It is located at a very close distance from the Sun, above the mid-plane. It is very well-studied in the literature.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 293.983 | 35.668 | – | -1.96 | -2.57 | – |
| Kharchenko et al. (2005) | 294.04 | 35.67 | – | -1.35 | -2.3 | – |
| Piskunov et al. (2008) | 294.04 | 35.668 | – | – | – | – |
| Kharchenko et al. (2013) | 294.075 | 35.66 | – | -0.83 | -1.97 | – |
| Kharchenko et al. (2016) | 294.07 | 35.658 | – | – | – | – |
| Loktin & Popova (2017) | 293.985 | 35.668 | – | -1.96 | -2.57 | – |
| Cantat-Gaudin et al. (2018) | 294.091 | 35.742 | 2.007 | -0.683 | -2.439 | – |
| Bica et al. (2019) | 293.985 | 35.67 | – | – | – | – |
| Soubiran et al. (2018) | 294.091 | 35.742 | – | – | – | -7.66 |
| Bossini et al. (2019) | 294.091 | 35.742 | – | – | – | – |
| Liu & Pang (2019) | 294.09 | 35.764 | 2.007 | -0.682 | -2.463 | – |
| Cantat-Gaudin et al. (2020) | 294.091 | 35.742 | 2.007 | -0.683 | -2.439 | – |
| Dias et al. (2021) | 294.109 | 35.751 | 2.007 | -0.653 | -2.419 | -9.391 |
| Tarricq et al. (2022) | 294.031 | 35.735 | 2.006 | -0.632 | -2.458 | – |
| He et al. (2022) | 294.142 | 35.747 | 2.011 | -0.65 | -2.456 | – |
| Just et al. (2023) | 294.07 | 35.658 | – | – | – | – |
| Qin et al. (2023) | 294.14 | 35.74 | 2.02 | -0.63 | -2.47 | -7.5 |
| Hunt & Reffert (2023) | 294.084 | 35.708 | 2.0 | -0.63 | -2.477 | -6.984 |
| Cavallo et al. (2024) | 294.177 | 35.842 | 2.013 | – | – | – |
| Hunt & Reffert (2024) | 294.084 | 35.708 | 2.0 | -0.63 | -2.477 | -6.984 |
| Zhang et al. (2024) | 294.084 | 35.708 | – | – | – | – |
| Alfonso et al. (2024) | 294.087 | 35.745 | 1.976 | -0.639 | -2.461 | – |
| Almeida et al. (2025) | 294.109 | 35.751 | – | – | – | – |
| UCC | 294.079 | 35.742 | 2.008 | -0.649 | -2.471 | -6.956 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.0, Dist=700.0, Age=8.37 |
| Kharchenko et al. (2005) | E(B-V)=0.0, Dist=700, logt=8.37 |
| Piskunov et al. (2008) | E(B-V)=0.0, Dist=700, logt=8.37, logMA=2.475 |
| Kharchenko et al. (2013) | E(B-V)=0.0, d=841.0, logt=8.39 |
| Kharchenko et al. (2016) | E(B-V)=0.0, d=841.0, logt=8.39 |
| Loktin & Popova (2017) | E(B-V)=0.861, Dist=921, logt=8.704 |
| Cantat-Gaudin et al. (2018) | dmode=491.3 |
| Soubiran et al. (2018) | dmode=491.3 |
| Bossini et al. (2019) | AV=0.0, Dist=8.38, logA=7.9, Fe/H=0.0 |
| Liu & Pang (2019) | Age=0.033, Z=0.25 |
| Cantat-Gaudin et al. (2020) | AVNN=0.0, DistPc=509.0, AgeNN=8.01 |
| Dias et al. (2021) | Av=0.141, Dist=492, logage=8.364, [Fe/H]=0.078 |
| Tarricq et al. (2022) | Dist=503, logAgeNN=8.02 |
| He et al. (2022) | A0=0.25, logAge=7.9 |
| Just et al. (2023) | logt=8.39, logmt=2.061 |
| Qin et al. (2023) | E(B-V)=0.1, m-M=8.7, logt=7.9 |
| Hunt & Reffert (2023) | AV50=0.138, diffAV50=0.728, MOD50=8.389, logAge50=8.1 |
| Cavallo et al. (2024) | AV50=0.47, dMod50=8.53, logAge50=7.92, [Fe/H]50=0.22 |
| Hunt & Reffert (2024) | MassJ=295.113, MassTot=415.293 |
| Zhang et al. (2024) | [Fe/H]ANN=0.08943, [Fe/H]MCMC=0.11485 |
| Alfonso et al. (2024) | AV=0.00164, MOD=8.53870, logAge=7.91409, Z=0.07906 |
| Almeida et al. (2025) | AV=0.141, Dist=492, logAge=8.364, MassRk=249.9 |
Search coordinates in Bayestar19