Type Ia supernova

Supernova

Supernova

Supernovae Sparked by Dark Matter in White Dwarfs

Supernovae Sparked by Dark Matter in White Dwarfs

How Supernovae Became the Basis of Observational Cosmology

How Supernovae Became the Basis of Observational Cosmology

Asymmetric Type-Ia Supernova Origin of W49B As Revealed from Spatially Resolved X-Ray Spectroscopic Study Ping Zhou1,2 and Jacco Vink1,3

Asymmetric Type-Ia Supernova Origin of W49B As Revealed from Spatially Resolved X-Ray Spectroscopic Study Ping Zhou1,2 and Jacco Vink1,3

1. Basic Properties of Supernovae During the Past Two Decades, There Has Occurred a Technological Break-Through in Astronomy

1. Basic Properties of Supernovae During the Past Two Decades, There Has Occurred a Technological Break-Through in Astronomy

Pos(GOLDEN2019)046 Model 6 Model May Be Inconsistent 6 Model Can Be Also Progenitors of Peculiar Sne Ia

Pos(GOLDEN2019)046 Model 6 Model May Be Inconsistent 6 Model Can Be Also Progenitors of Peculiar Sne Ia

Lecture 17 Type Ia Supernovae

Lecture 17 Type Ia Supernovae

SPECTROSCOPIC OBSERVATIONS of SN 2012Fr: a LUMINOUS, NORMAL TYPE Ia SUPERNOVA with EARLY HIGH-VELOCITY FEATURES and a LATE VELOCITY PLATEAU

SPECTROSCOPIC OBSERVATIONS of SN 2012Fr: a LUMINOUS, NORMAL TYPE Ia SUPERNOVA with EARLY HIGH-VELOCITY FEATURES and a LATE VELOCITY PLATEAU

Observational Properties of Thermonuclear Supernovae

Observational Properties of Thermonuclear Supernovae

A Supernova Is the Explosive Death of a Star. • Two Types Are Easily

A Supernova Is the Explosive Death of a Star. • Two Types Are Easily

Supernovae and Cosmology

Supernovae and Cosmology

Investigating Supernova Remnants

Investigating Supernova Remnants

Identifying Type Ia Supernovae in Extragalactic Spectra

Identifying Type Ia Supernovae in Extragalactic Spectra

A Faint Type of Supernova from a White Dwarf with a Helium-Rich Companion

A Faint Type of Supernova from a White Dwarf with a Helium-Rich Companion

Igniting a Standard Candle

Igniting a Standard Candle

Supernovae • Types Ib, Ic: No H Lines Due to Shell Loss (Type Ia Already Discussed) Type II: Plenty of H Left (Standard End Stage of SG)

Supernovae • Types Ib, Ic: No H Lines Due to Shell Loss (Type Ia Already Discussed) Type II: Plenty of H Left (Standard End Stage of SG)

11 Supernovae

11 Supernovae

CHAPTER 14 II Stellar Evolution

CHAPTER 14 II Stellar Evolution

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