학술논문

Ti-44 Gamma-Ray Emission Lines from SN1987A Reveal an Asymmetric Explosion
Document Type
Report
Source
Science Magazine. 348(6235)
Subject
Astrophysics
Language
English
ISSN
1095-9203
Abstract
In core-collapse supernovae, titanium-44 (Ti-44) is produced in the innermost ejecta, in the layer of material directly on top of the newly formed compact object. As such, it provides a direct probe of the supernova engine. Observations of supernova 1987A (SN1987A) have resolved the 67.87- and 78.32-kilo-electron volt emission lines from decay of Ti-44 produced in the supernova explosion. These lines are narrow and redshifted with a Doppler velocity of ~700 kilometers per second, direct evidence of large-scale asymmetry in the explosion.