Amanote Research

Amanote Research

    RegisterSign In

Evidence for Azimuthal Asymmetry in Be Star Winds

International Astronomical Union Colloquium
doi 10.1017/s0252921100071736
Full Text
Open PDF
Abstract

Available in full text

Date

January 1, 1999

Authors
Geraldine J. Peters
Publisher

Cambridge University Press (CUP)


Related search

Three-Dimensional Radiative Transfer in Clumped Hot Star Winds

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2012English

The Basic Physics of Hot-Star Winds

Symposium - International Astronomical Union
1994English

Transverse Single Spin and Azimuthal Asymmetries in Hadronic Collisions at STAR

EPJ Web of Conferences
AstronomyPhysics
2015English

Three-Component Modeling of C-Rich AGB Star Winds

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2003English

On the Onset of Galactic Winds in Quiescent Star Forming Galaxies

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2007English

Radiation-Accellerated Ions in Hot Star Winds: Heating and “Turbulence” Effects

Symposium - International Astronomical Union
1994English

Ultraviolet Observations, Stellar Winds, and Mass Loss for Be Stars

Symposium - International Astronomical Union
1982English

Alfven Wave–driven Proto–Neutron Star Winds Andr‐Process Nucleosynthesis

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2005English

The Be Star Φ Persei

Symposium - International Astronomical Union
1980English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2025 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy