August 27, 2025
Raven “Vampire” stars can use cosmic accomplices to devour star victims

Raven “Vampire” stars can use cosmic accomplices to devour star victims

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An illustration shows a white vampire dwarf that feeds from a sacrificial star, but the star lurked in the background brought her together. | Credit: CalTech/r. Injured (ipac)

For some time, astronomers have been cosmic vampires, dead stars that withdraw plasma hungry from sacrificial stars. New studies indicate that some of these cosmic fault in the form of a third star in their systems have accomplices, Renfields to their draculas and facilitate their fateful encounter.

These systems are known as cataclyysmic variables, and their occupants are white dwarfs, the type of star residue, which is left with masses around the sun, when they die.

The matter that has stolen their victims out of these white dwarfs stacked on the surfaces of the dead stars and finally prompted them to do and explore Supernova. Although the endings of catastrophic variables are quite well understood, this research suggests at least one new history of origin.

“Our results show a different formation channel for catastrophic variables,” said Kareem El-Badry, researcher by California Institute of Technology (CalTech), in a explanation. “Sometimes a lurking third star is the key.”

Lurking third stars are terrible matchmaker

The current consensus on catastrophic variables is that they form when two stars are brought together by a “joint envelope” of gas that is wrapped around them. This is known as “shared handling development”.

One of these two stars finally swells up as a red giant and paves up to 100 times its original size and swallows its outstanding companion. After this envelope, this star is swung together, it is ejected. The red giant is now a striped core, which is called a white dwarf with a companion star that is close enough so that the dead star removes it from its outer layers.

While many stars exist in binary files, triple-star systems are also common in the universe. This prompted El-Badry, CalTech Doctoral Cheyanne Shariat and her team to wonder how this process would have an impact on three stars.

To investigate this, the Duo of the Gaia Mission of the European Space Agency (ESA) turned. Before his latest retirement, Gaia pursued billions of stars to collect data that enables scientists to create a detailed 3D card of our cosmic back yard.

EL-Badry and Shariat found 50 catastrophic variables in triple-star systems, in which two stars are closely merged, while a third orbit pathways at a much greater distance.

A bright white ball that is connected by a lane made of orange smoke with a large orange ball

An illustration of the region that surrounds a feeding super massive black hole. | Credit: Robert Lea (created with Canva)

These results presented the duo that around 10% of catastrophic variables are found in three-star systems, a percentage that would be lower if lurking third stars had no role in creating cataclyysmic variables.

In order to confirm this connection, the astronomers carried out 2,000 simulations of hypothetical triple-star systems and observed the gravitational interactions between the three stars while the systems developed.

In 400 systems, cataclyysmic variables were born without the common envelope curve. In this 20% sample of the overall simulations, it was the third star that “put” the main ninemonian and forced it together.

“The severity of the third star causes the binary stars to have a super -centered orbit, and this forces the companion star closer to the white dwarf,” said Shariat. “The tidal forces derive energy and shrink and circulating the orbit. The star does not have to spiral through the common shell.”

A conical spaceship in the foreground, with a dense column of white light and gas in the background

The ESA mission GAIA shows an illustration that observes the Milky Way. | Credit: spaceship: ESA/ATG Medialab; Milky Way: Esa/Gaia/DPAC; CC BY-SA 3.0 IGO. Recognition: A. Moitinho.

But that wasn’t all. A joint envelope began in 60% of the simulated systems and was triggered by the third star.

In the remaining 20% of the simulations that formed together in a standard form without the third star forms.

The duo adapted your data to take a more realistic population of stars into account.

This is four times higher than the Gaia rehearsal. The team justifies that this is due to the fact that many third stars in these systems were either too difficult to see or were expelled from the system.

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The simulations carried out by EL-Badry and Shariat also enabled the team to predict the type of triple-star systems that form more catastrophic variables.

They found that with the help of a third star, white dwarfs rather feed on an outstanding companion with the help of a third star when the system begins with the third star, which is separated from the distance between earth and the sun over 100 times.

In fact, GAIA data seemed to show that three times systems with catastrophic variables tend to indicate wider organs.

“In the past 50 years, people have used the Model of Spiral-In-Evolutionary model of the spiral-in environment to explain the cataclyysmic variable education,” concluded El-Badry. “Nobody had noticed beforehand that this was largely done in three more!”

The team’s research was published in the Journal Publications of the Astronomical Society of the Pacific.

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