Super star cluster
Super star clusters are huge star clusters of very young large stars. They are thought to be precursors of globular clusters.[1] Their short-lived huge blue stars emit lots of UV radiation which ionises the surrounding gas. Examples are Westerlund 1 and 2 in the Milky Way, and R136 in the Larger Magellanic Cloud. Nearby galaxy NGC 1569 has two SSCs.
Super Star Cluster Media
- Grand star-forming region R136 in NGC 2070 (captured by the Hubble Space Telescope).jpg
R136 is an example of a super star cluster
- Westerlund 1.jpg
This image shows the star cluster "Westerlund 1" in infrared light as observed by the 2 Micron All-Sky Survey (2MASS). The field of view is approximately twice as large the Chandra image.*Scale: Image is 13 arcmin per side
- Star cluster RCW 38.jpg
New observations with ESO’s Very Large Telescope show the star cluster RCW 38 in all its glory. This image was taken during testing of the HAWK-I camera with the GRAAL adaptive optics system. It shows the cluster and its surrounding clouds of brightly glowing gas in exquisite detail, with dark tendrils of dust threading through the bright core of this young gathering of stars.
- Grand star-forming region R136 in NGC 2070 (captured by the Hubble Space Telescope).jpg
R136 (Located in the Tarantula Nebula)
- NGC 1722 NIRCam.jpg
NGC 1722 containing H72.97-69.39
- Ngc346.jpg
A Hubble Space Telescope (HST) image of NGC 346.
- NGC 1569.jpg
Galaxy NGC 1569 as imaged by the Hubble Space Telescope
- Starburst in a Dwarf Irregular Galaxy.jpg
Starburst in a Dwarf Irregular Galaxy
References
- ↑ Gallagher & Grebel (2002). "Extragalactic star clusters: speculations on the future". Extragalactic Star Clusters, IAU Symposium. 207: 207. arXiv:astro-ph/0109052. Bibcode:2002IAUS..207..745G.