Alessi 36
0.31
UTI
0.8
CN
1.0
Cdens
1.0
CC3
0.25
Clit
0.46
Cdup
Radius (P>50% members)
34.3 [arcmin]
- CN 0.8 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.25 Poorly studied
- Cdup 0.46 Possibly duplicate
Overview
Alessi 36 is a rich, very dense object of very high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied 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 | 106.61 | -37.644 | 3.605 | -9.662 | 7.082 | 15.355 |
| Hunt & Reffert | 2024 | 106.565 | -37.596 | 3.598 | -9.669 | 7.046 | 14.546 |
| Cavallo et al. | 2024 | 106.763 | -37.723 | 3.601 | â | â | â |
| Hunt & Reffert | 2023 | 106.565 | -37.596 | 3.598 | -9.669 | 7.046 | 14.546 |
| Bica et al. | 2019 | 106.588 | -37.487 | â | â | â | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | â | â | â | â | â | 100* | â | â |
| Cavallo et al. | 2024 | 0.28 | 0.62 | â | 21 | -0.030 | â | â | â |
| Hunt & Reffert | 2023 | 0.28 | 0.14 | 0.58 | 29 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Gold sample.