NGC 1893 explained
NGC 1893 |
Class: | Open cluster |
Dist Ly: | 3790abbr=onNaNabbr=on[1] |
Appmag V: | 7.5 |
Size V: | 11.0′ |
Age: | 4 Myr |
Names: | Cr 63, Mel 33, C0519+333, Lund 166, OCL 439, OCISM 101, Raab 24 |
NGC 1893 is an open cluster in the constellation Auriga. It is about 12,400 light years away. The star cluster is embedded in the Tadpole Nebula (HII region IC 410).
Images of the star cluster by the Chandra X-ray Observatory suggest that it contains approximately 4,600 young stellar objects.[2]
External links
Notes and References
- Kinematics in Young Star Clusters and Associations with Gaia DR2 . The Astrophysical Journal . 870 . 1 . 32. 2018 . 1807.02115 . 2019ApJ...870...32K . 10.3847/1538-4357/aaef8c . Kuhn . Michael A. . Hillenbrand . Lynne A. . Sills . Alison . Feigelson . Eric D. . Getman . Konstantin V. . 119328315 . free .
- Kuhn. Michael A.. Getman. Konstantin V.. Feigelson. Eric D.. The Spatial Structure of Young Stellar Clusters. Ii. Total Young Stellar Populations . The Astrophysical Journal. 802. 1. 2015. 60. 1538-4357. 10.1088/0004-637X/802/1/60. 1501.05300. 2015ApJ...802...60K. 119309858 .