No surviving evolved companions to the progenitor of supernova SN 1006
Jonay I. Gonzalez Hernandez, Pilar Ruiz-Lapuente, Hugo M. Tabernero,, David Montes, Ramon Canal, Javier Mendez, Luigi R. Bedin

TL;DR
This study searches for surviving stellar companions to the supernova SN 1006 and finds none, strongly suggesting that most Type Ia supernovae do not originate from the single-degenerate channel involving evolved companion stars.
Contribution
It provides the first comprehensive search for evolved companions to SN 1006, excluding giants and subgiants, thus constraining the progenitor scenarios of Type Ia supernovae.
Findings
No surviving giant or subgiant companions found near SN 1006
Less than 20% of Type Ia supernovae originate from the single-degenerate channel
Supports the dominance of the double-degenerate channel in Type Ia supernovae
Abstract
Type Ia supernovae are thought to occur as a white dwarf made of carbon and oxygen accretes sufficient mass to trigger a thermonuclear explosion. The accretion could occur slowly from an unevolved (main-sequence) or evolved (subgiant or giant) star, that being dubbed the single-degenerate channel, or rapidly as it breaks up a smaller orbiting white dwarf (the double- degenerate channel). Obviously, a companion will survive the explosion only in the single-degenerate channel. Both channels might contribute to the production of type Ia supernovae but their relative proportions still remain a fundamental puzzle in astronomy. Previous searches for remnant companions have revealed one possible case for SN 1572, though that has been criticized. More recently, observations have restricted surviving companions to be small, main-sequence…
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