Year: 2010
Type: conference-paper
Abstract: Observations of the explosions of Population III (Pop III) stars have the potential to teach us much about the formation and evolution of these zero‐metallicity objects. To realize this potential, we must tie observed emission to an explosion model, which requires accurate light curve and spectra calculations. Here, we discuss many of the pitfalls and problems involved in such models, presenting some preliminary results from radiation‐hydrodynamics simulations.
Source: AIP conference proceedings
DOI: 10.1063/1.3518894
Authors: Chris L. Fryer, Daniel J. Whalen, Lucy Frey, Daniel J. Whalen, Volker Bromm, Naoki Yoshida
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: green
OpenAlex ID: W2045867686