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- W3023644546 endingPage "2285" @default.
- W3023644546 startingPage "2253" @default.
- W3023644546 abstract "A range of astronomical data indicates that ancient supernovae created the galactic environment of the Sun and sculpted the physical properties of the interstellar medium near the heliosphere. In this paper, we review the characteristics of the local interstellar medium that have been affected by supernovae. The kinematics, magnetic field, elemental abundances, and configuration of the nearest interstellar material support the view that the Sun is at the edge of the Loop I superbubble, which has merged into the low-density Local Bubble. The energy source for the higher temperature X-ray-emitting plasma pervading the Local Bubble is uncertain. Winds from massive stars and nearby supernovae, perhaps from the Sco-Cen association, may have contributed radioisotopes found in the geologic record and galactic cosmic ray population. Nested supernova shells in the Orion and Sco-Cen regions suggest spatially distinct sites of episodic star formation. The heliosphere properties vary with the pressure of the surrounding interstellar cloud. A nearby supernova would modify this pressure equilibrium and thereby severely disrupt the heliosphere as well as the local interstellar medium." @default.
- W3023644546 created "2020-05-13" @default.
- W3023644546 creator A5017774929 @default.
- W3023644546 creator A5064620659 @default.
- W3023644546 date "2017-01-01" @default.
- W3023644546 modified "2023-10-02" @default.
- W3023644546 title "Effect of Supernovae on the Local Interstellar Material" @default.
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