4.6 Article

Dust driven mass loss from carbon stars as a function of stellar parameters I. A grid of solar-metallicity wind models

Rate this paper

The primary rating indicates the level of overall quality for the paper. Secondary ratings independently reflect strengths or weaknesses of the paper.

Find Funding. Review Successful Grants.

Explore over 25,000 new funding opportunities and over 6,000,000 successful grants.

Explore

Discover Peeref hubs

Discuss science. Find collaborators. Network.

Join a conversation