Palomar 6 [SEP] constellation
Palomar 6
Palomar 6 is a loose globular cluster in the constellation Ophiuchus that belongs to the halo of the Milky Way galaxy. 
First discovered on the National Geographic Society – Palomar Observatory Sky Survey plates by Robert G. Harrington and Fritz Zwicky,
It was catalogued as a globular cluster. One of four globulars known to contain a planetary nebula.
External links.
- Simbad reference data
- SEDS: Palomar 6, Capricornus Dwarf
have been obtained (beginning at 6 hours after the actual explosion), is the Type II SN 2013fs (iPTF13dqy) which was recorded 3 hours after the supernova event on 6 October 2013 by the Intermediate Palomar Transient Factory (iPTF). The star is located in a spiral galaxy named NGC 7610, 160 million light years away in the constellation of Pegasus.
On 20 September 2016, amateur astronomer Victor Buso from Rosario, Argentina was testing his telescope. When taking several photographs of galaxy NGC 613, Buso chanced upon