FSR 0406
(MWSC 3671)
0.69
UTI
0.82
CN
1.0
Cdens
0.62
CC3
0.5
Clit
1.0
Cdup
Radius (P>50% members)
2.9 [arcmin]
- CN 0.82 Rich
- Cdens 1.0 Very dense
- CC3 0.62 Intermediate quality
- Clit 0.5 Moderately studied
- Cdup 1.0 Unique
Overview
FSR 0406 is a rich, very dense object of intermediate C3 quality. Its parallax locates it at a close* distance, above the mid-plane, affected by very high extinction. It is catalogued as a young cluster (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~0.84 kpc) differs significantly from the median photometric distance (~7.08 kpc).
Note: This object shares a small percentage of members with 2 later reported entries. See table with shared members information.
Very distant
Very high extinction
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | β | 343.444 | 62.599 | 1.195 | -1.335 | -2.772 | -23.992 |
| Just et al. | 2023 | 343.422 | 62.597 | β | β | β | β |
| SΓ‘nchez et al. | 2020 | 343.45 | 62.612 | β | -1.275 | -2.608 | β |
| Kharchenko et al. | 2016 | 343.422 | 62.597 | β | β | β | β |
| Dias et al. | 2014 | 343.45 | 62.612 | β | -0.31 | -1.24 | β |
| Kharchenko et al. | 2013 | 343.428 | 62.6 | β | -0.76 | -3.28 | -23.7 |
| Kharchenko et al. | 2012 | 343.428 | 62.6 | β | -0.96 | -2.43 | β |
| Froebrich et al. | 2007 | 343.45 | 62.612 | β | β | β | β |
| Dias et al. | 2002 | 343.45 | 62.612 | β | -0.31 | -1.24 | β |
π‘ 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 | β | β | β | 20 | β | 604 | β | β |
| Kharchenko et al. | 2016 | 7.15 | 9.90 | β | 20 | β | β | β | β |
| Kharchenko et al. | 2013 | 7.15 | 9.90 | β | 20 | β | β | β | β |
| Kharchenko et al. | 2012 | 7.00 | 4.49 | β | 1000 | β | β | β | β |
| Dias et al. | 2002 | 7.00 | 4.49 | β | 1000 | β | β | β | β |
