ASCC 104
(MWSC 3147)
0.38
UTI
0.0
CN
0.23
Cdens
0.38
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members)
38.1 [arcmin]
- CN 0.0 Sparse
- Cdens 0.23 Very loose
- CC3 0.38 Low quality
- Clit 0.65 Moderately studied
- Cdup 1.0 Unique
Overview
ASCC 104 is a sparse, very loose object of low C3 quality. Its parallax locates it at a very close* distance, near the mid-plane, affected by moderate extinction. It is catalogued as a young cluster (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~0.41 kpc) differs significantly from the median photometric distance (~0.80 kpc).
Close
Moderate extinction
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 294.745 | 18.686 | 2.456 | 2.279 | -3.851 | -20.562 |
| Hunt & Reffert | 2023 | 294.696 | 18.619 | 2.461 | 2.372 | -3.77 | -11.532 |
| Just et al. | 2023 | 294.736 | 18.663 | â | â | â | â |
| Bica et al. | 2019 | 294.723 | 18.687 | â | â | â | â |
| Kharchenko et al. | 2016 | 294.736 | 18.663 | â | â | â | â |
| Dias et al. | 2014 | 294.721 | 18.69 | â | -0.99 | -3.22 | â |
| Kharchenko et al. | 2013 | 294.742 | 18.665 | â | -0.06 | -4.65 | -5.6 |
| Gozha et al. | 2012 | 294.721 | 18.69 | â | â | â | â |
| Piskunov et al. | 2008 | 294.714 | 18.692 | â | â | â | â |
| Kharchenko et al. | 2007 | 294.72 | 18.69 | â | 0.48 | â | -5.65 |
| Kharchenko et al. | 2005 | 294.72 | 18.69 | â | -0.09 | -4.65 | -5.65 |
| Dias et al. | 2002 | 294.721 | 18.69 | â | -0.09 | -4.65 | -6.68 |
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 | 2023 | 0.40 | 0.23 | 0.37 | 122 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 51 | â | 169 | â | â |
| Kharchenko et al. | 2016 | 0.77 | 1.03 | â | 51 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.77 | 1.03 | â | 51 | â | â | â | â |
| Gozha et al. | 2012 | 0.80 | â | â | 51 | â | 1514 | â | â |
| Piskunov et al. | 2008 | 0.80 | 1.02 | â | 51 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.80 | 1.02 | â | 51 | â | â | â | â |
| Dias et al. | 2002 | 0.80 | 1.02 | â | 51 | â | â | â | â |


Hunt & Reffert (2024)
Classified as a moving group.