NGC 2335
(MWSC 1100; FoF 2080; CMa19)
Summary
NGC 2335 is a rich, very dense object of high C3 quality. It is located at a relatively close distance from the Sun, near the mid-plane. It is very well-studied in the literature.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 106.704 | -10.028 | – | -0.91 | -3.18 | -3.59 |
| Chen et al. (2003) | 106.716 | -10.045 | – | – | – | – |
| Kharchenko et al. (2003) | 106.71 | -10.05 | – | 0.98 | -2.38 | – |
| Kharchenko et al. (2005) | 106.71 | -10.03 | – | 1.45 | -3.31 | – |
| Piskunov et al. (2007) | 106.706 | -10.027 | – | – | – | – |
| Kharchenko et al. (2007) | 106.71 | -10.03 | – | 0.25 | – | 8.7 |
| Piskunov et al. (2008) | 106.706 | -10.027 | – | – | – | – |
| Kharchenko et al. (2013) | 106.71 | -10.03 | – | 0.2 | -2.99 | 8.7 |
| Kharchenko et al. (2016) | 106.704 | -10.028 | – | – | – | – |
| Loktin & Popova (2017) | 106.71 | -10.027 | – | -1.9 | -2.647 | 8.7 |
| Cantat-Gaudin et al. (2018) | 106.69 | -10.023 | 0.585 | -0.784 | -0.642 | – |
| Liu & Pang (2019) | 106.7 | -10.014 | 0.571 | -0.791 | -0.654 | – |
| Cantat-Gaudin et al. (2020) | 106.69 | -10.023 | 0.585 | -0.784 | -0.642 | – |
| Dias et al. (2021) | 106.679 | -10.015 | 0.581 | -0.793 | -0.658 | – |
| Rain et al. (2021) | 106.69 | -10.023 | 0.585 | -0.784 | -0.642 | – |
| Santos-Silva et al. (2021) | 106.67 | -10.03 | 0.58 | -0.77 | -0.66 | – |
| Jaehnig et al. (2021) | 106.694 | -10.029 | 0.618 | -0.779 | -0.662 | – |
| Just et al. (2023) | 106.704 | -10.028 | – | – | – | – |
| Hunt & Reffert (2023) | 106.723 | -10.041 | 0.574 | -0.789 | -0.628 | 24.277 |
| Cavallo et al. (2024) | 106.675 | -10.017 | 0.582 | – | – | – |
| Hunt & Reffert (2024) | 106.723 | -10.041 | 0.574 | -0.789 | -0.628 | 24.277 |
| Almeida et al. (2025) | 106.679 | -10.015 | – | – | – | – |
| UCC | 106.688 | -10.03 | 0.579 | -0.798 | -0.634 | 23.85 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.393, Dist=1417.0, Age=8.21, [Fe/H]=-0.18 |
| Chen et al. (2003) | E(B-V)=0.393, HDis=1417, Age=0.16, [Fe/H]_1=-0.03 |
| Kharchenko et al. (2003) | E(B-V)=0.39, Dist=1408 |
| Kharchenko et al. (2005) | E(B-V)=0.39, Dist=1417, logt=8.08 |
| Piskunov et al. (2007) | E(B-V)=0.39, Dist=1417, logt=8.08, logM=2.135 |
| Piskunov et al. (2008) | E(B-V)=0.39, Dist=1417, logt=8.08, logM=2.85, logMA=2.889 |
| Kharchenko et al. (2013) | E(B-V)=0.416, d=1411.0, logt=8.2, [Fe/H]=-0.03 |
| Kharchenko et al. (2016) | E(B-V)=0.416, d=1411.0, logt=8.2 |
| Loktin & Popova (2017) | E(B-V)=0.395, Dist=1470, logt=8.232 |
| Cantat-Gaudin et al. (2018) | dmode=1629.8 |
| Liu & Pang (2019) | Age=0.355, Z=0.25 |
| Cantat-Gaudin et al. (2020) | AVNN=0.83, DistPc=1661.0, AgeNN=8.51 |
| Dias et al. (2021) | Av=1.48, Dist=1462, logage=7.812, [Fe/H]=-0.071 |
| Rain et al. (2021) | E(B-V)=0.39, Dist=1629.8, log(Age)=8.21, NBSS=0 |
| Santos-Silva et al. (2021) | AVPM=1.54, AVPf=1.24, DPM=1446, DPf=1413.0, AgeM=42.0, AgeF=60, [Fe/H]M=-0.09, [Fe/H]f=0.3 |
| Jaehnig et al. (2021) | dmode=1.603 |
| Just et al. (2023) | logt=8.2, logmt=2.67 |
| Hunt & Reffert (2023) | AV50=1.357, diffAV50=2.407, MOD50=11.011, logAge50=8.17 |
| Cavallo et al. (2024) | AV50=1.26, dMod50=11.19, logAge50=8.34, [Fe/H]50=0.56 |
| Hunt & Reffert (2024) | MassJ=984.961, MassTot=984.961 |
| Almeida et al. (2025) | AV=1.48, Dist=1462, logAge=7.812, MassRk=693.4 |
Search coordinates in Bayestar19