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.

Припис:

ESO/Callingham et al.

Про зображення

ID:eso1838a
Тип:Спостереження
Дата релізу [date]:19 листопада 2018 р. 17:00
Пов'язані релізи:eso1838
Розмір:1440 x 1440 px

Про об’єкт

Назва:Apep
Тип:Milky Way : Star : Grouping : Binary
Constellation:Norma
Категорія:Stars

Формати зображень

Великий JPEG
339,8 Кб

Координати

Position (RA):16 0 50.48
Position (Dec):-51° 42' 44.94"
Field of view:0.26 x 0.26 arcminutes
Орієнтація:Північ на -0.0° ліва від вертикалі

Кольори та фільтри

ДіапазонДовжина хвиліТелескоп
Інфрачервоний
IB
2.24 μmVery Large Telescope
NACO
Інфрачервоний
ArIII
8.9 μmVery Large Telescope
VISIR

 

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