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Literatur
Künstlerische Darstellung eines Gasrings Hamburger Sternwarte - Forschung: Bp-Sterne
Auswirkungen von Wind, Magnetfeld und Rotation bei heißen Sternen


Literaturangaben

Groote, D. & Hunger, K. (1976), Variable Shell Spectrum of σ Ori E,
Astronomy & Astrophysics, 52, S.303

Michaud, G., Charland, Y., Vauclair, S., Vauclair, G.(1976), Diffusion in main-sequence stars: Radiation forces, time scales, anomalies,
Astrophysical Journal 210, S.447

Shore, S.N. (1987), Stellar winds and magnetic fields in helium peculiar stars,
Astronomical Journal 94, S.731

Babel, J. (1995), Multi-component radiatively driven winds from A and B stars I: The metallic wind of a main sequence A star,
Astronomy & Astrophysics, 301, S.823

Groote, D. & Hunger, K. (1997), Fractionated stellar wind - the example of σ Orionis E,
Astronomy & Astrophysics, 319, S.250

Hunger, K. & Groote, D. (1999), Fractionated stellar wind and the H/He abundance anomalies in Bp stars,
Astronomy & Astrophysics, 351, S.554

Smith, M.A. & Groote, D. (2001), Wind circulation in selected rotating magnetic early-B stars,
Astronomy & Astrophysics, (im Druck)

Townsend R., Owocki S. (2004), in A Rigidly Rotating Magnetosphere Model for the Circumstellar Environments of Magnetic OB Stars, ASP Conference Series, (im Druck)

ud'Doula A., Townsend R., Owocki S. (2004), in Centrifugal Breakout of Magnetically Torqued Line-Driven Stellar Winds, ASP Conference Series, (im Druck)



Friday, 08-Oct-2004 15:25:51 CEST | D.Groote