Relativistic Atomic Structure of Au IV and the Os Isoelectronic Sequence: Opacity Data for Kilonova Ejecta

Relativistic Atomic Structure of Au IV and the Os Isoelectronic Sequence: Opacity Data for Kilonova Ejecta

Direct detection of gravitational waves (GWs) on 17 August 2017, propagating from a binary neutron star merger, or a “kilonova”, opened the era of multimessenger astronomy. The ejected material from neutron star mergers, or “kilonova”, is a good candidate for optical and near infrared follow-up obse...

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Bibliographic Details
Main Authors: Zahra Sadat Taghadomi, Yier Wan, Alicia Flowers, Phillip Stancil, Brendan McLaughlin, Steven Bromley, Joan Marler, Chad Sosolik, Stuart Loch
Format: Article
Language:English
Published: MDPI AG 2022-09-01
Series:Atoms
Subjects:
atomic data
neutron stars
Online Access:https://www.mdpi.com/2218-2004/10/3/94

Internet

https://www.mdpi.com/2218-2004/10/3/94

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