Abundance tomography of type Ia supernovae

被引：0

作者：

Stehle, M ^{[1
]}

Mazzali, PA ^{[1
]}

Benetti, S ^{[1
]}

Hillebrandt, W ^{[1
]}

机构：

[1] Max Planck Inst Astrophys, D-85741 Garching, Germany

来源：

1604-2004: Supernovae as Cosmological Lighthouses | 2005年 / 342卷

关键词：

MODELS;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Analysis of early time spectra of type la supernovae is presented. "Abundance Tomography" is explained as a method to derive detailed abundance distribution of the supernova (SN) ejecta. Results from the application of this method to SN 2002bo are shown and conclusions on the explosion mechanism are drawn.

引用

页码：393 / 396

页数：4

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