FSR 0338
(MWSC 3570)
0.59
UTI
0.6
CN
0.65
Cdens
0.62
CC3
0.55
Clit
1.0
Cdup
Radius (P>50% members)
2.6 [arcmin]
- CN 0.6 Moderately populated
- Cdens 0.65 Moderately dense
- CC3 0.62 Intermediate quality
- Clit 0.55 Moderately studied
- Cdup 1.0 Unique
Overview
FSR 0338 is a moderately populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a large* distance, above the mid-plane, affected by very high extinction. It is catalogued as a very massive, intermediate-age cluster (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~6.14 kpc) differs significantly from the median photometric distance (~14.65 kpc).
Extremely distant
Very high extinction
Very massive
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 327.927 | 55.315 | 0.163 | -3.536 | -3.217 | â |
| He et al. | 2023 | 327.927 | 55.319 | 0.166 | -3.548 | -3.227 | â |
| Just et al. | 2023 | 327.927 | 55.309 | â | â | â | â |
| Bica et al. | 2019 | 327.929 | 55.329 | â | â | â | â |
| Kharchenko et al. | 2016 | 327.927 | 55.309 | â | â | â | â |
| Dias et al. | 2014 | 327.933 | 55.329 | â | -3.8 | -7.37 | â |
| Kharchenko et al. | 2013 | 327.933 | 55.313 | â | -6.26 | -4.22 | â |
| Kharchenko et al. | 2012 | 327.933 | 55.313 | â | -6.26 | -4.22 | â |
| Froebrich et al. | 2007 | 327.933 | 55.329 | â | â | â | â |
| Dias et al. | 2002 | 327.933 | 55.329 | â | -6.26 | -4.22 | â |
đĄ 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 |
|---|---|---|---|---|---|---|---|---|---|
| He et al. | 2023 | 6.46 | 5.40 | â | 794 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 126 | â | 5508 | â | â |
| Kharchenko et al. | 2016 | 14.65 | 6.45 | â | 126 | â | â | â | â |
| Kharchenko et al. | 2013 | 14.65 | 6.45 | â | 126 | â | â | â | â |
| Kharchenko et al. | 2012 | 14.65 | 6.45 | â | 126 | â | â | â | â |
| Dias et al. | 2002 | 14.65 | 6.45 | â | 126 | â | â | â | â |
