Ultraviolet spectropolarimetric diagnostics of hot star magnetospheres
Author:
Funder
National Aeronautics and Space Administration
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://link.springer.com/content/pdf/10.1007/s10509-022-04097-8.pdf
Reference127 articles.
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2. Ababakr, K.M., Oudmaijer, R.D., Vink, J.S.: A statistical spectropolarimetric study of Herbig Ae/Be stars. Mon. Not. R. Astron. Soc. 472(1), 854–868 (2017). https://doi.org/10.1093/mnras/stx1891. 1707.08408 [astro-ph.SR]
3. Abt, H.A., Levato, H.: Spectral types in the Orion OB1 association. Publ. Astron. Soc. Pac. 89, 797–802 (1977). https://doi.org/10.1086/130230
4. Adams, F.C., Laughlin, G.: A dying universe: the long-term fate and evolution of astrophysical objects. Rev. Mod. Phys. 69(2), 337–372 (1997). https://doi.org/10.1103/RevModPhys.69.337. astro-ph/9701131 [astro-ph]
5. Babel, J., Montmerle, T.: X-ray emission from Ap-Bp stars: a magnetically confined wind-shock model for IQ Aur. Astron. Astrophys. 323, 121–138 (1997)
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