Coils of Apep

The VISIR instrument on ESO’s VLT captured this stunning image of a newly-discovered massive binary star system. Nicknamed Apep after an ancient Egyptian deity, it could be the first gamma-ray burst progenitor to be found in our galaxy.

Apep’s stellar winds have created the dust cloud surrounding the system, which consists of a binary star with a fainter companion. With 2 Wolf-Rayet stars orbiting each other in the binary, the serpentine swirls surrounding Apep are formed by the collision of two sets of powerful stellar winds, which create the spectacular dust plumes seen in the image.

The reddish pinwheel in this image is data from the VISIR instrument on ESO’s Very Large Telescope (VLT), and shows the spectacular plumes of dust surrounding Apep. The blue sources at the centre of the image are a triple star system — which consists of a binary star system and a companion single star bound together by gravity. Though only two star-like objects are visible in the image, the lower source is in fact an unresolved binary Wolf-Rayet star. The triple star system was captured by the NACOadaptive optics instrument on the VLT.

Mynd/Myndskeið:

ESO/Callingham et al.

Um myndina

Auðkenni:eso1838a
Tegund:Athuganir
Útgáfudagur:Nóv 19, 2018, 17:00 CET
Tengdar fréttatilkynningar:eso1838
Stærð:1440 x 1440 px

Um fyrirbærið

Nafn:Apep
Tegund:Milky Way : Star : Grouping : Binary
Constellation:Norma
Flokkur:Stars

Myndasnið

Stór JPEG
339,8 KB

Hnit

Position (RA):16 0 50.48
Position (Dec):-51° 42' 44.94"
Field of view:0.26 x 0.26 arcminutes
Stefna:Norður er -0.0° vinstri frá lóðréttu

Litir og síur

TíðnisviðBylgjulengdSjónauki
Innrautt
IB
2.24 μmVery Large Telescope
NACO
Innrautt
ArIII
8.9 μmVery Large Telescope
VISIR

 

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