Two stars orbit each other within an enormous dusty disk in the U Monocerotis system, illustrated here. When the stars are farthest from each other, they funnel material from the disk’s inner edge. At this time, the primary star is slightly obscured by the disk from our perspective. The primary star, a yellow supergiant, expands and contracts. The smaller secondary star is thought to maintain its own disk of material, which likely powers an outflow of gas that emits X-rays. Credits: NASA’s Goddard Space Flight Center/Chris Smith (USRA/GESTAR) Download high-resolution video and images from NASA’s Scientific Visualization Studio
Astronomers have painted their best picture yet of an RV Tauri variable, a rare type of stellar binary where two stars — one approaching the end of its life ...
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