Teutsch 42
(MCM 23; MCM2005b 23; MWSC 3132)
0.57
UTI
0.48
CN
0.4
Cdens
0.75
CC3
0.6
Clit
1.0
Cdup
Stellar density (N50/rad)
2.0 [N/pc2]
- CN 0.48 Poorly populated
- Cdens 0.4 Loose
- CC3 0.75 High quality
- Clit 0.6 Moderately studied
- Cdup 1.0 Unique
Overview
Teutsch 42 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a large* distance, near the mid-plane, affected by very high extinction. It is catalogued as a very young cluster, but with a large variance across recent sources for the mass parameter (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~6.44 kpc) differs significantly from the median photometric distance (~2.00 kpc).
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 292.553 | 18.537 | 0.155 | -3.105 | -5.884 | â |
| Celli et al. | 2024 | 292.555 | 18.536 | â | â | â | â |
| Just et al. | 2023 | 292.548 | 18.531 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 292.554 | 18.535 | 0.182 | -3.116 | -5.83 | â |
| Cantat-Gaudin & Anders | 2020 | 292.554 | 18.535 | 0.182 | -3.116 | -5.83 | â |
| Cantat-Gaudin et al. | 2018 | 292.554 | 18.535 | 0.182 | -3.116 | -5.83 | â |
| Kharchenko et al. | 2016 | 292.548 | 18.531 | â | â | â | â |
| Kharchenko et al. | 2013 | 292.554 | 18.533 | â | -2.59 | -6.94 | â |
| Morales et al. | 2013 | 292.555 | 18.537 | â | â | â | â |
| Kronberger et al. | 2006 | 292.555 | 18.536 | â | â | â | â |
| Mercer et al. | 2005 | 292.555 | 18.538 | â | â | â | â |
| Dias et al. | 2002 | 292.554 | 18.536 | â | -1.96 | -5.06 | 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 | 2.0 | 8.24 | â | 1 | â | 246 | â | â |
| Celli et al. | 2024 | â | â | â | 1 | â | 480 | â | â |
| Just et al. | 2023 | â | â | â | 1 | â | 13 | â | â |
| Cantat-Gaudin & Anders | 2020 | 4.73 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 4.73 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 2.00 | 8.58 | â | 1 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.00 | 8.58 | â | 1 | â | â | â | â |
| Morales et al. | 2013 | 6.66 | â | â | 3 | â | â | â | â |
| Kronberger et al. | 2006 | 1.60 | 7.90 | â | 32 | â | â | â | â |
| Dias et al. | 2002 | 1.60 | 7.90 | â | 32 | â | â | â | â |
MOCA


Mercer et al. (2005)
Association of stars. Detected using no magnitude cut. Detected in 2MASS catalog with our algorithm. Appears in 2MASS images.
Morales et al. (2013)
Classified as morphological type 'OC1' (totally exposed cluster still physically associated with gas). Morphological flag: exposed cluster, without submm emission.