ASCC 36
(MWSC 1151)
- CN 0.0 Sparse
- Cdens 0.34 Loose
- CC3 0.12 Very low quality
- Clit 0.62 Moderately studied
- Cdup 1.0 Unique
Overview
ASCC 36 is a sparse, loose object of very low C3 quality. Its parallax locates it at a close distance, below the mid-plane. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is moderately studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | – | 108.688 | -21.054 | 1.01 | -2.251 | 1.972 | 18.79 |
| Hunt & Reffert | 2024 | 108.623 | -21.101 | 1.014 | -2.242 | 2.001 | 16.047 |
| Cavallo et al. | 2024 | 108.669 | -21.053 | 1.018 | – | – | – |
| Hunt & Reffert | 2023 | 108.623 | -21.101 | 1.014 | -2.242 | 2.001 | 16.047 |
| Just et al. | 2023 | 108.62 | -21.121 | – | – | – | – |
| Bica et al. | 2019 | 108.628 | -21.124 | – | – | – | – |
| Kharchenko et al. | 2016 | 108.62 | -21.121 | – | – | – | – |
| Kharchenko et al. | 2013 | 108.625 | -21.123 | – | -2.76 | 0.75 | – |
| Piskunov et al. | 2008 | 108.623 | -21.115 | – | – | – | – |
| Kharchenko et al. | 2005 | 108.63 | -21.12 | – | -2.15 | -0.87 | – |
| Dias et al. | 2002 | 108.629 | -21.12 | – | -1.89 | 0.25 | – |
💡 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | – | – | – | – | – | 67* | – | – |
| Cavallo et al. | 2024 | 0.99 | 0.35 | – | 85 | -0.290 | – | – | – |
| Hunt & Reffert | 2023 | 0.94 | 0.17 | 0.37 | 127 | – | – | – | – |
| Just et al. | 2023 | – | – | – | 214 | – | 46 | – | – |
| Kharchenko et al. | 2016 | 0.81 | 0.00 | – | 214 | – | – | – | – |
| Kharchenko et al. | 2013 | 0.81 | 0.00 | – | 214 | – | – | – | – |
| Piskunov et al. | 2008 | 0.75 | 0.00 | – | 324 | – | – | – | – |
| Kharchenko et al. | 2005 | 0.75 | 0.00 | – | 324 | – | – | – | – |
| Dias et al. | 2002 | 0.75 | 0.00 | – | 324 | – | – | – | – |
💡 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.
(*): indicates that this parameter is
assigned more than one value in the corresponding reference.
