NGC 3036
(MWSC 1719; ESO 126 27)
0.24
UTI
0.0
CN
0.07
Cdens
0.25
CC3
0.44
Clit
1.0
Cdup
Radius (P>50% members)
7.9 [arcmin]
- CN 0.0 Sparse
- Cdens 0.07 Very loose
- CC3 0.25 Low quality
- Clit 0.44 Poorly studied
- Cdup 1.0 Unique
Overview
NGC 3036 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate* distance, below the mid-plane. It is catalogued as a metal-poor, intermediate-age cluster (see Parameters). It is poorly studied in the literature. (*): The parallax distance estimate (~3.09 kpc) differs significantly from the median photometric distance (~1.20 kpc).
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | – | 147.296 | -62.624 | 0.324 | -6.77 | 4.976 | 5.405 |
| Just et al. | 2023 | 147.311 | -62.666 | – | – | – | – |
| Bica et al. | 2019 | 147.329 | -62.663 | – | – | – | – |
| Kharchenko et al. | 2016 | 147.311 | -62.666 | – | – | – | – |
| Kharchenko et al. | 2013 | 147.315 | -62.67 | – | -9.76 | 4.68 | 11.8 |
| Piskunov et al. | 2008 | 147.315 | -62.67 | – | – | – | – |
| Kharchenko et al. | 2005 | 147.31 | -62.67 | – | -7.43 | -1.25 | – |
| Dias et al. | 2002 | 147.317 | -62.672 | – | -4.47 | 2.09 | 11.78 |
💡 Note: The UCC values are estimated from its identified members.
| Reference | Year | Dist [kpc] | Av [mag] | DAv [mag] | Age [Myr] | [Fe/H] [dex] | Mass [Msun] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Just et al. | 2023 | – | – | – | 977 | – | 33 | – | – |
| Kharchenko et al. | 2016 | 1.27 | 1.29 | – | 977 | – | – | – | – |
| Kharchenko et al. | 2013 | 1.27 | 1.29 | – | 977 | -0.714 | – | – | – |
| Piskunov et al. | 2008 | 1.20 | 1.24 | – | 407 | – | – | – | – |
| Kharchenko et al. | 2005 | 1.20 | 1.24 | – | 407 | – | – | – | – |
| Dias et al. | 2002 | 1.20 | 1.24 | – | 407 | -0.714 | – | – | – |
💡 Note: The parameters are sometimes transformed from their original values to match the format of the columns shown here, see FAQ. The columns DAv, Bfr, BSS correspond to differential extinction, binary fraction, and blue stragglers, respectively. BSS values can be listed as fractions or integers.
