NGC2264
Sergison et al (2013)Mayne et al (2007)
NGC2264 was used as a fiducial cluster with an assumed age of 3Myrs in Mayne et al (2007).
This cluster also shows an R-C gap, as seen in the CMD, when our data are supplemented by the photometry of the 90% confidence proper motion members from Mendoza V. & Gomez (1980). We provide a note on how this catalogue was created and the catalogue itself.
Paper | Table | Description | Link |
| Sergison et al (2013) | 2 | EW[Li], Veiling, RVs and Hα parameters | ASCII |
| Spectra | gzipped ASCII tarball | ||
| Mayne et al (2007) | 8 | Full BVI catalogue | ASCII |
| 9 | Periodic variable stars from Dahm & Simon (2005) | ASCII | |
| 10 | X-ray sources from Flaccomio et al (1999) | ASCII | |
| 11 | Hα sources from Lamm et al (2004) | ASCII |