German astronomers uncover three new hydrogen-deficient pre-white dwarfs

Using the X-shooter instrument at ESO’s Very Large Telescope (VLT), German astronomers have detected three new pre-white dwarfs, which turned out to be strongly hydrogen-deficient. The discovering was reported in a analysis paper revealed December 20 on the pre-print server arXiv.

White dwarfs (WDs) are stellar cores left behind after a star has exhausted its nuclear gas. Due to their excessive gravity, they’re identified to have atmospheres of both pure hydrogen or pure helium. However, a small fraction of WDs exhibits traces of heavier components.

Although WDs have a comparatively small dimension, similar to that of the Earth, they’re a number of million occasions extra large than our planet. Pre-white dwarfs (PWDs) are a number of occasions bigger and slated to shrink in dimension, finally turning into WDs inside about a number of thousand years.

Now, a crew of astronomers led by Klaus Werner of the University of Tübingen in Germany, stories the discovering of three new PWDs with extraordinarily low hydrogen mass fraction.

“We have detected three new hydrogen-deficient (H < 0.001 mass fraction) pre-white dwarfs with helium-dominated atmospheres,” the researchers wrote within the paper.

The largest of the three newfound PWDs, designated GSC 08265, is about half the dimensions of the solar. The star, which is situated some 5,000 mild years away, has an efficient temperature of about 72,000 Okay and its mass is estimated to be 0.53 photo voltaic lots.

The astronomers observe that GSC 08265 is a PG1159 star within the earliest pre-white dwarf section. The so-called PG 1159 stars are precursors of the DO white dwarfs or DA white dwarfs, retaining some hydrogen of their envelope, named after their prototype.

One of the celebs reported within the research, named Gaia DR3 52, turned out to be a scorching subdwarf of spectral sort O(He). It has a radius of about 0.23 photo voltaic radii, whereas its mass is round 0.52 photo voltaic lots. The star, situated roughly 7,400 mild years away, has an efficient temperature of about 90,000 Okay.

The third newfound PWD is UCAC4 108—at a distance of some 5,700 mild years. The star is about 3 times smaller than the solar and its mass is estimated to be almost certainly about 0.8 photo voltaic lots. Werner’s crew has categorized UCAC4 108 as a scorching subdwarf of spectral sort CO-sdO, with an efficient temperature of fifty,000 Okay.

Summing up the outcomes, the authors of the paper underline that each one the three PWDs are strongly hydrogen-deficient and have nitrogen abundance at a degree of six occasions larger than that of the solar.

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