Astronomy and Astrophysics – Astrophysics
Scientific paper
2007-04-10
AIP Conf.Proc.937:51-57,2007
Astronomy and Astrophysics
Astrophysics
Highlights of invited talk at Aspen conference: "Supernova 1987A: 20 Years After -- Supernovae & Gamma-Ray Bursters"
Scientific paper
10.1063/1.2803617
The reverse shock of supernova remnant (SNR) 1987A emits in H-alpha and Ly-alpha, and comes in two flavors: surface and interior. The former is due to direct, impact excitation of hydrogen atoms crossing the shock, while the latter is the result of charge transfer reactions between these atoms and slower, post-shock ions. Interior and surface emission are analogous to the broad- and narrow-line components observed in Balmer-dominated SNRs. I summarize a formalism to derive line intensities and ratios in these SNRs, as well as a study of the transition zone in supernova shocks; I include an appendix where I derive in detail the ratio of broad to narrow H-alpha emission. Further study of the reverse shock emission from SNR 1987A will allow us to predict when it will vanish and further investigate the origins of the interior emission.
No associations
LandOfFree
The Reverse Shock of SNR 1987A does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The Reverse Shock of SNR 1987A, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Reverse Shock of SNR 1987A will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-672530