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Dr. Cunningham on White Dwarf Atmospheres and Accretion
Dr. Cunningham's findings throw fresh light on the enigmatic heavy-element pollution in white dwarf atmospheres. With the direct evidence from X-rays and the newly deduced accretion rates, the research reshapes our understanding of the processes at play in these ancient stellar remnants and suggests a need for refined models to fully capture the complexities unfolding in these stars.
White Dwarf Pollution: A significant number of white dwarf stars possess atmospheres tainted by heavy elements. These elements, intriguingly, should vanish from sight in a relatively short time due to gravitational settling.
Accretion Hypothesis: The presence of these heavy elements has long been thought to signify ongoing accretion (a process where matter accumulates onto a central body) of debris, possibly remnants of asteroids, comets, or even large planets. This theory gains strength from certain observations of debris discs and transiting planetary fragments near some white dwarfs.
Indirect Evidence: While these metals in a white dwarf's atmosphere hint towards accretion, they don't provide direct evidence. Relying on them to infer accretion rates or deduce the composition of the debris has its challenges and heavily leans on models of how these elements move and mix within the white dwarf's atmosphere.
X-ray Discovery from G29–38: Dr. Cunningham's breakthrough was the notable detection of X-rays emanating from a metal-polluted white dwarf named G29–38. This discovery allows for a more direct measure of the accretion rate, which turns out to be independent of the atmospheric models previously relied upon.
Accretion Rate: From these X-ray observations, they determined an instantaneous accretion rate. This rate surpasses previous estimations based on studying the white dwarf's surface heavy element concentrations.
Implications for Modelling: The higher-than-expected accretion rate might indicate that there's more happening beneath the visible layers of the white dwarf than currently understood. The mention of "convective overshoot" suggests that models may need to account for more vigorous mixing processes.
Low Plasma Temperature: They recorded a plasma temperature of around
0.5 ±0.2 keV 0.5±0.2keV, which backs up a theory suggesting that white dwarfs with low accretion rates are bombarded by incoming debris.
https://doi.org/10.1038/s41586-021-04300-w
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By Catarina CunhaDr. Cunningham's findings throw fresh light on the enigmatic heavy-element pollution in white dwarf atmospheres. With the direct evidence from X-rays and the newly deduced accretion rates, the research reshapes our understanding of the processes at play in these ancient stellar remnants and suggests a need for refined models to fully capture the complexities unfolding in these stars.
White Dwarf Pollution: A significant number of white dwarf stars possess atmospheres tainted by heavy elements. These elements, intriguingly, should vanish from sight in a relatively short time due to gravitational settling.
Accretion Hypothesis: The presence of these heavy elements has long been thought to signify ongoing accretion (a process where matter accumulates onto a central body) of debris, possibly remnants of asteroids, comets, or even large planets. This theory gains strength from certain observations of debris discs and transiting planetary fragments near some white dwarfs.
Indirect Evidence: While these metals in a white dwarf's atmosphere hint towards accretion, they don't provide direct evidence. Relying on them to infer accretion rates or deduce the composition of the debris has its challenges and heavily leans on models of how these elements move and mix within the white dwarf's atmosphere.
X-ray Discovery from G29–38: Dr. Cunningham's breakthrough was the notable detection of X-rays emanating from a metal-polluted white dwarf named G29–38. This discovery allows for a more direct measure of the accretion rate, which turns out to be independent of the atmospheric models previously relied upon.
Accretion Rate: From these X-ray observations, they determined an instantaneous accretion rate. This rate surpasses previous estimations based on studying the white dwarf's surface heavy element concentrations.
Implications for Modelling: The higher-than-expected accretion rate might indicate that there's more happening beneath the visible layers of the white dwarf than currently understood. The mention of "convective overshoot" suggests that models may need to account for more vigorous mixing processes.
Low Plasma Temperature: They recorded a plasma temperature of around
0.5 ±0.2 keV 0.5±0.2keV, which backs up a theory suggesting that white dwarfs with low accretion rates are bombarded by incoming debris.
https://doi.org/10.1038/s41586-021-04300-w