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1992
White dwarf stars represent the most common endpoint of stellar evolution. In fact, about 90% of all stars will end up as white dwarfs. Their high temperatures and low luminosities imply that they are small — only about the size of the Earth (R e = 0.009R⊙). The mean radius for white dwarfs is R = 0.01 R⊙ (see the first table).
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White dwarf stars represent the most common endpoint of stellar evolution. In fact, about 90% of all stars will end up as white dwarfs. Their high temperatures and low luminosities imply that they are small — only about the size of the Earth (R e = 0.009R⊙). The mean radius for white dwarfs is R = 0.01 R⊙ (see the first table).
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Pulsar Condition in White Dwarf Stars
Nature, 1968According to the recently proposed “astronomical sandglass model” of the pulsed radio sources1 a pulsar is a neutron star at the critical mass limit for gravitational instability. Any loss of stability resulting in incipient collapse is quickly restored by the remaining nuclear resources, which, it was assumed, can still generate thermal pulses of ...
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Brain and other central nervous system tumor statistics, 2021
Ca-A Cancer Journal for Clinicians, 2021Kimberly D Miller +2 more
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American Cancer Society's report on the status of cancer disparities in the United States, 2021
Ca-A Cancer Journal for Clinicians, 2022Farhad Islami +2 more
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Ecology and impacts of white-nose syndrome on bats
Nature Reviews Microbiology, 2021Joseph R Hoyt +2 more
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Suppression of cooling by strong magnetic fields in white dwarf stars
Nature, 2014G. Valyavin +20 more
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Breast cancer statistics, 2015: Convergence of incidence rates between black and white women
Ca-A Cancer Journal for Clinicians, 2016Carol E Desantis +2 more
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Breast cancer statistics, 2019
Ca-A Cancer Journal for Clinicians, 2019Carol E Desantis, Jiemin, Mia M Gaudet
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