Spectroscopic Modeling of Luminous Transients Powered by H-rich and He-rich Circumstellar Interaction

In this study, we perform detailed spectroscopic modeling to analyze the interaction of circumstellar material (CSM) with ejecta in both hydrogen-rich and hydrogen-poor superluminous supernovae (SLSNe), by systematically varying properties such as the CSM density, composition, and geometry to explor...

وصف كامل

التفاصيل البيبلوغرافية
الحاوية / القاعدة:	The Astrophysical Journal
المؤلفون الرئيسيون:	Gururaj A. Wagle, Emmanouil Chatzopoulos, Michael J. Baer
التنسيق:	مقال
اللغة:	الإنجليزية
منشور في:	IOP Publishing 2024-01-01
الموضوعات:	Radiative transfer Supernovae Circumstellar shells Stellar-interstellar interactions Monte Carlo methods Transient sources
الوصول للمادة أونلاين:	https://doi.org/10.3847/1538-4357/ad93d7

مواد مشابهة

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