Stellar Classification of White Dwarfs

In summary, the Yerkes Classification System was an older system for categorizing white dwarf stars based on surface temperature, but has since been replaced by a newer system that takes into account both surface temperature and spectral type. Diagrams of DQ, DZ, and DC stars on the HR Diagram can be found online.
  • #1
piareround
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OK recently I found a really old table stars based on partally on Yerkes Classification system with a small section on white dwarf stars. It has the stars organized into groups labeled DO, DA, DB, DF, DG, DK, and DM. However, I remember that the current classification system for white dwarf stars as primarily DO, DA, DB, DQ, DZ, DC, DX.

First, Has anyone heard of the first classification system? If so why where the letters changed? What happened?

Second, I really have trouble visualizing DQ, DZ, and DC on the HR diagram compared to the other white dwarfs. Does anyone have pictures of DQ, DZ, or DC stars on the HR Diagram?
 
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  • #2
The first classification system you are referring to is known as the Yerkes Classification System, which was developed in the early twentieth century and is no longer used today. The letters DO, DA, DB, DF, DG, DK, and DM were used to denote different types of stars based on their surface temperature. The current classification system for white dwarf stars (DO, DA, DB, DQ, DZ, DC, DX) was developed later and uses different letters to denote different types of stars based on a combination of surface temperature and spectral type. As for your second question, you can find diagrams of DQ, DZ, and DC stars on the HR Diagram online. For example, this website has a diagram that shows the locations of these stars: https://www.astronomynotes.com/starprop/s11.htm.
 

1. What is the definition of a white dwarf?

A white dwarf is a small, dense, and hot star that is the remnant core of a low-mass star. It is primarily composed of carbon and oxygen and has a radius comparable to that of the Earth, but with a mass equivalent to that of the Sun.

2. How are white dwarfs classified?

White dwarfs are classified based on their surface temperature and composition. They are divided into three main groups: DA, DB, and DO. DA white dwarfs have a hydrogen-rich atmosphere, DB white dwarfs have a helium-rich atmosphere, and DO white dwarfs have a mixture of hydrogen and helium in their atmosphere.

3. What is the temperature range of a white dwarf?

The temperature of a white dwarf can range from about 4,000 Kelvin to over 100,000 Kelvin. The hottest white dwarfs are also the youngest, as they cool over time.

4. How do white dwarfs form?

White dwarfs are formed when a low-mass star (less than 8 times the mass of the Sun) runs out of nuclear fuel and begins to collapse under its own gravity. This causes the core to become extremely hot and dense, eventually becoming a white dwarf.

5. Can white dwarfs support life?

No, white dwarfs are too small and dense to support life. In fact, they have extremely high surface gravity, making them inhospitable to any form of life as we know it. Additionally, their high temperatures and lack of a stable energy source make it impossible for any complex biological processes to occur.

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