Mass Loss of Stars on the Asymptotic Giant Branch

Höfner, S., & Olofsson, H. (2018). Mass Loss of Stars on the Asymptotic Giant Branch: Mechanisms, Models and Measurements. Astronomy and Astrophysics Review, 017-0106.

Type

Journal article

Intellectual base

Primary research

Year

2018

DOI

10.1007/s00159-017-0106-5

Link

https://doi.org/10.1007/s00159-017-0106-5

Cited by

1 citation across 1 artifact.

Domain-specific

• Stellar Wind
  • The solar wind is the supersonic expansion of the Sun's hot, magnetized corona; winds of hot massive stars are accelerated mainly by radiation interacting with spectral lines; winds of cool asymptotic-giant-branch stars depend on pulsation, dust formation, and radiation pressure on grains coupled to gas.

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Registry ID ref:88acdc7df493 · see in the full table