Tycho Brahe's 1572 supernova as a standard type Ia explosion revealed from its light echo spectrum
Oliver Krause, Masaomi Tanaka, Tomonori Usuda, Takashi Hattori, Miwa, Goto, Stephan Birkmann, Ken'ichi Nomoto

TL;DR
This study analyzes a light echo from Tycho Brahe's 1572 supernova to classify it as a normal Type Ia supernova, providing insights into its explosion mechanism and confirming its similarity to typical SNe Ia.
Contribution
First spectroscopic analysis of SN 1572 from a light echo, confirming it as a normal Type Ia supernova and revealing asphericity in its explosion.
Findings
SN 1572 is classified as a normal SN Ia.
Presence of high-velocity Ca II IR feature indicating asphericity.
Spectroscopic data obtained more than four centuries after explosion.
Abstract
Type Ia supernovae (SNe Ia) are thermonuclear explosions of white dwarf stars in close binary systems. They play an important role as cosmological distance indicators and have led to the discovery of the accelerated expansion of the Universe. Among the most important unsolved questions are how the explosion actually proceeds and whether accretion occurs from a companion or via the merging of two white dwarfs. Tycho Brahe's supernova of 1572 (SN 1572) is thought to be one of the best candidates for a SN Ia in the Milky Way. The proximity of the SN 1572 remnant has allowed detailed studies, such as the possible identification of the binary companion, and provides a unique opportunity to test theories of the explosion mechanism and the nature of the progenitor. The determination of the yet unknown exact spectroscopic type of SN 1572 is crucial to relate these results to the diverse…
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