NGC 1893
(MWSC 516)
Summary
NGC 1893 is a rich, very dense object of 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.
This object shares a small percentage of members with 2 later reported entries.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dambis (1999) | 80.683 | 33.412 | – | – | – | – |
| Dias et al. (2002) | 80.683 | 33.412 | – | -0.35 | -3.97 | -4.56 |
| Chen et al. (2003) | 80.674 | 33.388 | – | -1.3 | 0.21 | -4.7 |
| Kharchenko et al. (2003) | 80.68 | 33.41 | – | -0.45 | -4.72 | – |
| Kharchenko et al. (2005) | 80.68 | 33.41 | – | 0.35 | -4.37 | -2.25 |
| Piskunov et al. (2007) | 80.671 | 33.41 | – | – | – | – |
| Kharchenko et al. (2007) | 80.68 | 33.41 | – | 0.2 | – | -2.25 |
| Piskunov et al. (2008) | 80.671 | 33.41 | – | – | – | – |
| Kharchenko et al. (2012) | 80.707 | 33.43 | – | 2.25 | -5.65 | -9.17 |
| Kharchenko et al. (2013) | 80.707 | 33.43 | – | 2.25 | -5.65 | -9.2 |
| Kharchenko et al. (2016) | 80.698 | 33.43 | – | – | – | – |
| Loktin & Popova (2017) | 80.7 | 33.43 | – | 0.468 | -1.594 | -9.2 |
| Cantat-Gaudin et al. (2018) | 80.724 | 33.444 | 0.267 | -0.231 | -1.41 | – |
| Soubiran et al. (2018) | 80.724 | 33.444 | – | – | – | -3.72 |
| Cantat-Gaudin et al. (2020) | 80.724 | 33.444 | 0.267 | -0.231 | -1.41 | – |
| Dias et al. (2021) | 80.753 | 33.443 | 0.26 | -0.216 | -1.435 | – |
| Rain et al. (2021) | 80.724 | 33.444 | 0.267 | -0.231 | -1.41 | – |
| Jaehnig et al. (2021) | 80.724 | 33.447 | 0.283 | -0.205 | -1.396 | – |
| Just et al. (2023) | 80.698 | 33.43 | – | – | – | – |
| Hunt & Reffert (2023) | 80.702 | 33.426 | 0.295 | -0.29 | -1.398 | 21.59 |
| Cavallo et al. (2024) | 80.737 | 33.453 | 0.298 | – | – | – |
| Celli et al. (2024) | 80.724 | 33.444 | – | – | – | – |
| Hunt & Reffert (2024) | 80.702 | 33.426 | 0.295 | -0.29 | -1.398 | 21.59 |
| Almeida et al. (2025) | 80.753 | 33.443 | – | – | – | – |
| UCC | 80.726 | 33.446 | 0.3 | -0.283 | -1.411 | 20.89 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dambis (1999) | E_B-V_=0.501, DM0=12.1, log_age_=6.4 |
| Dias et al. (2002) | E(B-V)=0.56, Dist=3500.0, Age=6.18 |
| Chen et al. (2003) | HDis=3280, Age=0.01 |
| Kharchenko et al. (2003) | E(B-V)=0.4, Dist=3333 |
| Kharchenko et al. (2005) | E(B-V)=0.4, Dist=3280, logt=6.82 |
| Piskunov et al. (2007) | E(B-V)=0.4, Dist=3280, logt=6.82, logM=2.703 |
| Piskunov et al. (2008) | E(B-V)=0.4, Dist=3280, logt=6.82, logM=3.48, logMA=3.461 |
| Kharchenko et al. (2012) | E(B-V)=0.949, d=3300.0, logt=6.55 |
| Kharchenko et al. (2013) | E(B-V)=0.949, d=3300.0, logt=6.55 |
| Kharchenko et al. (2016) | E(B-V)=0.949, d=3300.0, logt=6.55 |
| Loktin & Popova (2017) | E(B-V)=0.578, Dist=3268, logt=7.047 |
| Cantat-Gaudin et al. (2018) | dmode=3373.5 |
| Soubiran et al. (2018) | dmode=3373.5 |
| Cantat-Gaudin et al. (2020) | AVNN=1.28, DistPc=3222.0, AgeNN=6.64 |
| Dias et al. (2021) | Av=1.686, Dist=3019, logage=7.04, [Fe/H]=-0.104 |
| Rain et al. (2021) | E(B-V)=0.56, Dist=3373.5, log(Age)=6.18, NBSS=0 |
| Jaehnig et al. (2021) | dmode=3.472 |
| Just et al. (2023) | logt=6.55, logmt=2.844 |
| Hunt & Reffert (2023) | AV50=1.522, diffAV50=2.449, MOD50=12.347, logAge50=7.322 |
| Cavallo et al. (2024) | AV50=1.3, dMod50=12.01, logAge50=7.32, [Fe/H]50=0.19 |
| Celli et al. (2024) | Age=4.4, Mc=1205.1 |
| Hunt & Reffert (2024) | MassJ=1537.91, MassTot=1537.91 |
| Almeida et al. (2025) | AV=1.686, Dist=3019, logAge=7.04, MassRk=743.5 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| OC 0293 | 15.8 | 80.71 | 33.43 | 0.32 | -0.32 | -1.43 | 38.23 | 0.0 |
| SAI 48 | 3.7 | 80.86 | 33.49 | 0.3 | -0.15 | -1.26 | 40.83 | 0.11 |
