Alexander Heger

Professor

MONASH UNIVERSITY

Australia

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About

Professor Alexander Heger is a faculty member at Monash University in Australia. His research focuses on astrophysics, particularly in the areas of supernovae, the evolution of primordial stars, and nucleosynthesis processes. Recent articles authored by Professor Heger explore topics such as neutrino-driven explosions, metal-poor stars, and X-ray bursts. His work contributes to advancing the understanding of stellar evolution and explosive phenomena in the universe.

Articles (12)

Year:

2023

Year:

2023

Year:

2022

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2022

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2022

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2022

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2021

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2021

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2021

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2021

Year:

2021

Year:

2021

Collaborators (8)

Tyrone Woods

Assistant Professor

University of Manitoba

CANADA

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Wako Aoki

教授/Professor

自然科学研究機構国立天文台/National Astronomical Observatory of Japan

JAPAN

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Teresa Kurtukian-Nieto

Profesor de Investigación

SPAIN

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Hidetoshi Yamaguchi

Lecturer

University of Tokyo

JAPAN

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Athira Menon

Lecturer and Science Fellow

Columbia University in the City of New York

UNITED STATES

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Nadezda Smirnova

University of Bordeaux

FRANCE

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Bernhard Mueller

Associate Professor

MONASH UNIVERSITY

AUSTRALIA

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Daniel James Whalen

Academic, Senior Lecturer, Senior Lecturer

University of Portsmouth

UNITED KINGDOM

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Alexander Heger

Research Interests

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About

Articles (12)

Light Curves of Type IIP Supernovae from Neutrino-driven Explosions of Red Supergiants Obtained by a Semianalytic Approach

A metal-poor star with abundances from a pair-instability supernova

The Regulated NiCu Cycles with the New 57Cu(p,γ)58Zn Reaction Rate and Its Influence on Type I X-Ray Bursts: the GS 1826–24 Clocked Burster

Measurement of 19F(p, γ)20Ne reaction suggests CNO breakout in first stars

Long-term Evolution of Postexplosion Helium-star Companions of Type Iax Supernovae

Impact of the New 65As(p,γ)66Se Reaction Rate on the Two-proton Sequential Capture of 64Ge, Weak GeAs Cycles, and Type I X-Ray Bursts Such as the Clocked Burster GS 1826−24

Advancement of Photospheric Radius Expansion and Clocked Type-I X-Ray Burst Models with the New Mg22(α,p)Al25 Reaction Rate Determined at the Gamow Energy

X-ray burst ignition location on the surface of accreting X-ray pulsars: can bursts preferentially ignite at the hotspot?

On the Evolution of Supermassive Primordial Stars in Cosmological Flows

Self-consistent 3D Supernova Models From −7 Minutes to +7 s: A 1-bethe Explosion of a ∼19 M ⊙ Progenitor

Supernova 1987A: 3D Mixing and Light Curves for Explosion Models Based on Binary-merger Progenitors

The Pair-instability Mass Gap for Black Holes

Collaborators (8)

Tyrone Woods

Wako Aoki

Teresa Kurtukian-Nieto

Hidetoshi Yamaguchi

Athira Menon

Nadezda Smirnova

Bernhard Mueller

Daniel James Whalen

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