HSC 415
0.08
UTI
0.36
CN
0.28
Cdens
0.75
CC3
0.0
Clit
0.28
Cdup
Radius (P>50% members)
56.7 [arcmin]
- CN 0.36 Poorly populated
- Cdens 0.28 Loose
- CC3 0.75 High quality
- Clit 0.0 Rarely studied
- Cdup 0.28 Possibly duplicate
Overview
HSC 415 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a very close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
â ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.
Very close
Low extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 275.291 | 21.651 | 3.271 | -1.157 | -7.368 | -17.263 |
| Cavallo et al. | 2024 | 275.064 | 21.612 | 3.266 | â | â | â |
| Hunt & Reffert | 2023 | 275.25 | 22.772 | 3.262 | -1.141 | -7.382 | -21.632 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| Cavallo et al. | 2024 | 0.32 | 0.78 | â | 18 | -0.040 | â | â | â |
| Hunt & Reffert | 2023 | 0.30 | 0.13 | 0.40 | 33 | â | â | â | â |
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.