FSR 1595
(MWSC 1976)
0.79
UTI
0.68
CN
1.0
Cdens
0.75
CC3
0.75
Clit
1.0
Cdup
Stellar density (N50/rad)
18.0 [N/pc2]
- CN 0.68 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
FSR 1595 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a large distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 176.77 | -62.631 | 0.198 | -6.77 | 1.367 | -0.969 |
| Hunt & Reffert | 2024 | 176.768 | -62.636 | 0.215 | -6.735 | 1.332 | -6.003 |
| Cavallo et al. | 2024 | 176.742 | -62.611 | 0.214 | â | â | â |
| Hunt & Reffert | 2023 | 176.768 | -62.636 | 0.215 | -6.735 | 1.332 | -6.003 |
| Just et al. | 2023 | 176.744 | -62.646 | â | â | â | â |
| Spina et al. | 2021 | 176.77 | -62.64 | 0.178 | -6.796 | 1.389 | â |
| Cantat-Gaudin et al. | 2020 | 176.771 | -62.639 | 0.179 | -6.779 | 1.373 | â |
| Cantat-Gaudin & Anders | 2020 | 176.771 | -62.639 | 0.179 | -6.779 | 1.373 | â |
| Soubiran et al. | 2018 | 176.771 | -62.639 | â | â | â | -11.85 |
| Cantat-Gaudin et al. | 2018 | 176.771 | -62.639 | 0.179 | -6.779 | 1.373 | â |
| Kharchenko et al. | 2016 | 176.744 | -62.646 | â | â | â | â |
| Dias et al. | 2014 | 176.771 | -62.637 | â | -8.46 | -2.82 | â |
| Kharchenko et al. | 2013 | 176.752 | -62.65 | â | -3.48 | -1.28 | 0.0 |
| Froebrich et al. | 2007 | 176.771 | -62.637 | â | â | â | â |
| Dias et al. | 2002 | 176.771 | -62.637 | â | -3.48 | -1.28 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 4.59 | 2.65 | 2.53 | 25 | 0.044 | 832 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 843(1) | â | â |
| Cavallo et al. | 2024 | 3.77 | 3.24 | â | 89 | -0.040 | â | â | â |
| Hunt & Reffert | 2023 | 4.06 | 2.92 | 2.53 | 48 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 2 | â | 822 | â | â |
| Spina et al. | 2021 | 4.76 | â | â | 692 | 0.128(20) | â | â | â |
| Cantat-Gaudin et al. | 2020 | 5.40 | 2.45 | â | 692 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 4.81 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 4.81 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 4.81 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 4.42 | 2.65 | â | 2 | â | â | â | â |
| Kharchenko et al. | 2013 | 4.42 | 2.65 | â | 2 | â | â | â | â |
| Dias et al. | 2002 | 4.42 | 2.65 | â | 2 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Wood sample.