FSR 1415
(SAI 93; MWSC 1526)
0.20
UTI
0.0
CN
0.01
Cdens
0.12
CC3
0.44
Clit
1.0
Cdup
Radius (P>50% members)
6.4 [arcmin]
- CN 0.0 Sparse
- Cdens 0.01 Very loose
- CC3 0.12 Very low quality
- Clit 0.44 Poorly studied
- Cdup 1.0 Unique
Overview
FSR 1415 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a large* distance, below the mid-plane, affected by very high extinction. It is catalogued as an old cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~9.29 kpc) differs significantly from the median photometric distance (~3.50 kpc).
Distant
Very high extinction
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | – | 130.102 | -44.719 | 0.108 | -2.483 | 2.56 | 73.084 |
| Just et al. | 2023 | 130.09 | -44.722 | – | – | – | – |
| Bica et al. | 2019 | 130.096 | -44.735 | – | – | – | – |
| Kharchenko et al. | 2016 | 130.09 | -44.722 | – | – | – | – |
| Kharchenko et al. | 2013 | 130.095 | -44.725 | – | -6.16 | 4.93 | – |
| Glushkova et al. | 2010 | 130.091 | -44.734 | – | – | – | – |
| Froebrich et al. | 2007 | 130.104 | -44.736 | – | – | – | – |
| Dias et al. | 2002 | 130.092 | -44.734 | – | 0.39 | 3.56 | – |
💡 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 | – | – | – | 1778 | – | 223 | – | – |
| Kharchenko et al. | 2016 | 3.47 | 6.13 | – | 1778 | – | – | – | – |
| Kharchenko et al. | 2013 | 3.47 | 6.13 | – | 1778 | – | – | – | – |
| Glushkova et al. | 2010 | 3.53 | 5.80 | – | 1778 | – | – | – | – |
| Dias et al. | 2002 | 3.53 | 5.80 | – | 1778 | – | – | – | – |
💡 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.
