Shorlin 2
(MWSC 1887)
0.03
UTI
0.0
CN
0.04
Cdens
0.12
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
6.7 [arcmin]
- CN 0.0 Sparse
- Cdens 0.04 Very loose
- CC3 0.12 Very low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
Shorlin 2 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 moderate extinction. It is catalogued as a very young cluster (see Parameters). It is rarely studied in the literature.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Distant
Moderate extinction
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 166.344 | -61.246 | 0.199 | -6.357 | 1.447 | â |
| Just et al. | 2023 | 166.38 | -61.252 | â | â | â | â |
| Kharchenko et al. | 2016 | 166.38 | -61.252 | â | â | â | â |
| Kharchenko et al. | 2013 | 166.387 | -61.255 | â | -5.25 | -2.21 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Just et al. | 2023 | â | â | â | 1 | â | 357 | â | â |
| Kharchenko et al. | 2016 | 4.13 | 1.16 | â | 1 | â | â | â | â |
| Kharchenko et al. | 2013 | 4.13 | 1.16 | â | 1 | â | â | â | â |
Dias et al. (2002)
Asterism (Turner, D. G. 2012, private communication)