VLT view of binary system R Aquarii from 2012
R Aquarii is a so-called “symbiotic binary”, comprising two stars surrounded by a large, dynamic cloud of gas (a nebula). Systems like this contain two stars in an unequal and complex relationship. R Aquarii is made up of one hot white dwarf and one red giant. The red giant is losing matter to its small companion and occasionally ejecting matter in weird spurts, loops and trails, forming the intriguing shapes seen here.
There is a lot going on between the performers in this cosmic double act. The red giant is a variable star, with a brightness that changes by a factor of 750 every year and three weeks. The faint nebula is named Cederblad 211 and is thought to be the result of a violent nova 250 years ago. Also visible is a narrow, vertical, S-shaped feature, with blobs of superheated material moving outward at tremendous speeds of 600 to 850 kilometres per second.
R Aquarii was also imaged 15 years ago — and several times in the intervening period — to track its ongoing activity. The system is very dynamic and complex, and has expanded and evolved significantly in recent years (an image from 1997 can be seen here, and a comparison between the two is available here).Mynd/Myndskeið:
|Útgáfudagur:||Des 10, 2018, 06:00 CET|
|Stærð:||1873 x 1166 px|
|Tegund:||Milky Way : Star : Grouping : Binary|
|Position (RA):||23 43 49.60|
|Position (Dec):||-15° 17' 11.67"|
|Field of view:||5.99 x 3.73 arcminutes|
|Stefna:||Norður er 0.1° vinstri frá lóðréttu|
Litir og síur
|500 nm||Very Large Telescope|
|372 nm||Very Large Telescope|
|656 nm||Very Large Telescope|