NGC 2414
(MWSC 1263)
Summary
NGC 2414 is a rich, very dense object of very high C3 quality. It is located at a large distance from the Sun, above the mid-plane. It is very well-studied in the literature.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dambis (1999) | 113.3 | -15.453 | – | – | – | – |
| Dias et al. (2002) | 113.3 | -15.453 | – | -1.87 | -0.26 | 67.14 |
| Chen et al. (2003) | 113.344 | -15.417 | – | -1.61 | 2.03 | 64.5 |
| Kharchenko et al. (2003) | 113.31 | -15.45 | – | -2.83 | 0.85 | – |
| Kharchenko et al. (2005) | 113.31 | -15.45 | – | -2.42 | 1.65 | 65.6 |
| Kharchenko et al. (2007) | 113.29 | -15.45 | – | 0.12 | – | 65.6 |
| Piskunov et al. (2008) | 113.303 | -15.45 | – | – | – | – |
| Kharchenko et al. (2013) | 113.287 | -15.455 | – | -1.79 | 0.0 | 65.6 |
| Kharchenko et al. (2016) | 113.281 | -15.453 | – | – | – | – |
| Loktin & Popova (2017) | 113.295 | -15.452 | – | -1.178 | -1.613 | 65.6 |
| Cantat-Gaudin et al. (2018) | 113.293 | -15.449 | 0.162 | -1.41 | 1.426 | – |
| Soubiran et al. (2018) | 113.293 | -15.449 | – | – | – | 194.97 |
| Dias et al. (2019) | 113.3 | -15.453 | 0.171 | -1.393 | 1.46 | 194.97 |
| Cantat-Gaudin et al. (2020) | 113.293 | -15.449 | 0.162 | -1.41 | 1.426 | – |
| Dias et al. (2021) | 113.29 | -15.449 | 0.161 | -1.409 | 1.414 | – |
| Rain et al. (2021) | 113.293 | -15.449 | 0.162 | -1.41 | 1.426 | – |
| Jaehnig et al. (2021) | 113.293 | -15.449 | 0.189 | -1.422 | 1.422 | – |
| Just et al. (2023) | 113.281 | -15.453 | – | – | – | – |
| Hunt & Reffert (2023) | 113.293 | -15.452 | 0.179 | -1.416 | 1.454 | 57.457 |
| Cavallo et al. (2024) | 113.285 | -15.44 | 0.18 | – | – | – |
| Celli et al. (2024) | 113.293 | -15.449 | – | – | – | – |
| Hunt & Reffert (2024) | 113.293 | -15.452 | 0.179 | -1.416 | 1.454 | 57.457 |
| Almeida et al. (2025) | 113.29 | -15.449 | – | – | – | – |
| UCC | 113.297 | -15.448 | 0.179 | -1.419 | 1.443 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dambis (1999) | E_B-V_=0.547, DM0=12.5, log_age_=7.2 |
| Dias et al. (2002) | E(B-V)=0.508, Dist=3455.0, Age=6.976 |
| Chen et al. (2003) | HDis=3455, Age=0.0 |
| Kharchenko et al. (2003) | E(B-V)=0.51, Dist=3448 |
| Kharchenko et al. (2005) | E(B-V)=0.56, Dist=2888, logt=6.94 |
| Piskunov et al. (2008) | E(B-V)=0.56, Dist=2888, logt=6.94, logMA=2.366 |
| Kharchenko et al. (2013) | E(B-V)=0.583, d=2874.0, logt=7.27 |
| Kharchenko et al. (2016) | E(B-V)=0.583, d=2874.0, logt=7.27 |
| Loktin & Popova (2017) | E(B-V)=0.543, Dist=2906, logt=6.922 |
| Cantat-Gaudin et al. (2018) | dmode=5249.2 |
| Soubiran et al. (2018) | dmode=5249.2 |
| Dias et al. (2019) | E(B-V)=0.53, Dist=4467, logAge=7.233, Z=0.007 |
| Cantat-Gaudin et al. (2020) | AVNN=1.48, DistPc=5273.0, AgeNN=7.25 |
| Dias et al. (2021) | Av=1.672, Dist=3624, logage=7.752, [Fe/H]=-0.198 |
| Rain et al. (2021) | E(B-V)=0.5, Dist=5249.2, log(Age)=6.97, NBSS=0 |
| Jaehnig et al. (2021) | dmode=5.204 |
| Just et al. (2023) | logt=7.27, logmt=2.646 |
| Hunt & Reffert (2023) | AV50=1.684, diffAV50=0.714, MOD50=13.54, logAge50=7.317 |
| Cavallo et al. (2024) | AV50=1.49, dMod50=12.84, logAge50=7.81, [Fe/H]50=0.15 |
| Celli et al. (2024) | Age=17.8, Mc=1242.5 |
| Hunt & Reffert (2024) | MassJ=2390.42, MassTot=2496.04 |
| Almeida et al. (2025) | AV=1.672, Dist=3624, logAge=7.752, MassRk=1090.8 |
Search coordinates in Bayestar19