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Unusual laser emissions beaming from the Ant Nebula suggest that it is home to a hidden double-star system and that one of the companion stars is nearing the end of its life.
When stars similar to our sun start to die, they become dense white dwarf stars and then expel their outer layers to form an interstellar cloud of gas and dust known as a planetary nebula. Any lingering gas close to the center would soon fall back onto the star, leaving the surrounding area empty. However, that is not what has been observed around the Ant Nebula, according to a statement from the European Space Agency (ESA).
Menzel - Structure - Gas - Object - Center
"When we observe Menzel 3, we see an amazingly intricate structure made up of ionized gas, but we cannot see the object in its center producing this pattern," Isabel Aleman, lead author of a new study detailing the observations and a researcher at the University of Sao Paulo, in Brazil, and the Leiden Observatory, in the Netherlands, said in the statement. "Thanks to the sensitivity and wide wavelength range of the Herschel observatory, we detected a very rare type of emission called hydrogen recombination line laser emission, which provided a way to reveal the nebula's structure and physical conditions."
This image shows possible evolutionary pathways for stars of different masses. Sunlike stars can be seen swelling into red giants before releasing their outer gas, creating colorful nebulas around a collapsed core called a white dwarf.
Observations - Density - Gas - Ant - Nebula
Specifically, the new observations show that the density of the laser-emitting gas surrounding the Ant Nebula is 10,000 times higher than that of the gas seen in typical planetary nebulas. This finding suggests that the Ant Nebula is actually home to two stars,...
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