IC 2944
(MWSC 1957)
0.95
UTI
0.75
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
2.7 [arcmin]
- CN 0.75 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
IC 2944 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate* distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is very well-studied in the literature.
(*): The parallax distance estimate (~2.55 kpc) differs significantly from the median photometric distance (~1.79 kpc).
Note: This object shares a large percentage of members with 3 later reported entries. See table with shared members information.
Relatively close
Low extinction
Near-solar metallicity
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 174.565 | -63.366 | 0.393 | -6.09 | 0.659 | 0.021 |
| Hunt & Reffert | 2024 | 174.599 | -63.381 | 0.391 | -6.08 | 0.694 | 5.006 |
| Cavallo et al. | 2024 | 174.55 | -63.364 | 0.39 | â | â | â |
| Hunt & Reffert | 2023 | 174.599 | -63.381 | 0.391 | -6.08 | 0.694 | 5.006 |
| Just et al. | 2023 | 174.045 | -62.946 | â | â | â | â |
| Jaehnig et al. | 2021 | 174.837 | -63.246 | 0.494 | -5.937 | 0.79 | â |
| Loktin & Popova | 2017 | 174.585 | -63.373 | â | -5.16 | -2.39 | -0.9 |
| Kharchenko et al. | 2016 | 174.045 | -62.946 | â | â | â | â |
| Dias et al. | 2014 | 174.583 | -63.373 | â | -5.16 | -2.39 | â |
| Kharchenko et al. | 2013 | 174.052 | -62.95 | â | -7.04 | -1.07 | -0.9 |
| Gozha et al. | 2012 | 174.583 | -63.373 | â | â | â | â |
| Piskunov et al. | 2008 | 174.031 | -62.951 | â | â | â | â |
| Kharchenko et al. | 2007 | 174.58 | -63.37 | â | 0.24 | â | â |
| van den Bergh | 2006 | 174.585 | -63.373 | â | â | â | â |
| Kharchenko et al. | 2005 | 174.03 | -62.95 | â | -6.2 | -1.17 | â |
| Kharchenko et al. | 2003 | 174.03 | -62.95 | â | -5.41 | -0.43 | â |
| Chen et al. | 2003 | 174.213 | -63.059 | â | -5.39 | 0.04 | -1.0 |
| Dias et al. | 2002 | 174.583 | -63.373 | â | -5.16 | -2.39 | -2.41 |
| Dambis | 1999 | 174.585 | -63.373 | 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 | 308* | â | â |
| Cavallo et al. | 2024 | 2.48 | 1.00 | â | 15 | -0.060 | â | â | â |
| Hunt & Reffert | 2023 | 2.37 | 1.11 | 1.36 | 4 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 2 | â | 414 | â | â |
| Jaehnig et al. | 2021 | 2.03* | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.79 | 0.99 | â | 7 | â | â | â | â |
| Kharchenko et al. | 2016 | 2.10 | 1.35 | â | 2 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.10 | 1.35 | â | 2 | â | â | â | â |
| Gozha et al. | 2012 | 1.79 | â | â | 7 | â | 2692 | â | â |
| Piskunov et al. | 2008 | 1.79 | 0.99 | â | 8 | â | â | â | â |
| van den Bergh | 2006 | 1.79 | 0.99 | â | 7 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.79 | 0.99 | â | 8 | â | â | â | â |
| Kharchenko et al. | 2003 | 1.79 | 0.99 | â | â | â | â | â | â |
| Chen et al. | 2003 | 1.79 | â | â | 0 | â | â | â | â |
| Dias et al. | 2002 | 1.79 | 0.99 | â | 7 | â | â | â | â |
| Dambis | 1999 | 2.07 | 1.10 | â | 3 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Silver sample.