Mass Loss from Hot Massive Stars.

Puls, J., Vink, J. S., & Najarro, F. (2008). Mass Loss from Hot Massive Stars. Astronomy and Astrophysics Review, 209-325.

Type

Journal article

Intellectual base

Primary research

Year

2008

DOI

10.1007/s00159-008-0015-8

Link

https://doi.org/10.1007/s00159-008-0015-8

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.

Verification

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Registry ID ref:7a098c2900d7 · see in the full table