Stellar mergers as the origin of magnetic massive stars
About ten per cent of 'massive' stars (those of more than 1.5 solar masses) have strong, large-scale surface magnetic fields1-3. It has been suggested that merging of main-sequence and pre-main-sequence stars could produce such strong fields4,5, and the predicted fraction of merged massive...
Κύριοι συγγραφείς: | Schneider, FRN, Ohlmann, ST, Podsiadlowski, P, Röpke, FK, Balbus, SA, Pakmor, R, Springel, V |
---|---|
Μορφή: | Journal article |
Γλώσσα: | English |
Έκδοση: |
Springer Nature
2019
|
Παρόμοια τεκμήρια
-
Rejuvenation of stellar mergers and the origin of magnetic fields in massive stars
ανά: Schneider, F, κ.ά.
Έκδοση: (2016) -
The slow merger of massive stars
ανά: Ivanova, N, κ.ά.
Έκδοση: (2003) -
The Slow Merger of Massive Stars
ανά: Ivanova, N, κ.ά.
Έκδοση: (2002) -
The slow merger of massive stars: Merger types and post-merger evolution
ανά: Ivanova, N, κ.ά.
Έκδοση: (2002) -
Massive Star Mergers: Induced Mixing and Nucleosynthesis
ανά: Ivanova, N, κ.ά.
Έκδοση: (2001)