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arXiv · 1904.06600

High-Resolution X-ray Imaging Studies of Neutron Stars, Pulsar Wind Nebulae and Supernova Remnants

Samar Safi-Harb·Elena Amato·Eric V. Gotthelf·Satoru Katsuda·Manami Sasaki·Yasunobu Uchiyama·Naomi Tsuji·Benson Guest
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Abstract

Supernova remnants serve as nearby laboratories relevant to many areas in Astrophysics, from stellar and galaxy evolution to extreme astrophysics and the formation of the heavy elements in the Universe. The Chandra X-ray mission has enabled a giant leap forward in studying both SNRs and their compact stellar remnants on sub-arcsecond scale. However, such high-resolution imaging studies have been mostly limited to the nearby and/or relatively bright objects. There is no question that we are missing a large population, especially in external galaxies. Within our own Galaxy, we are presented with new fundamental questions related to neutron stars' diversity, kicks, relativistic winds and the way these objects interact with, and impact, their host environments. In this white paper, we highlight some of the breakthroughs to be achieved with future X-ray missions (such as the proposed AXIS probe) equipped with sub-arcsecond imaging resolution and an order of magnitude improvement in sensitivity.

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Samar Safi-Harb, Elena Amato, Eric V. Gotthelf, Satoru Katsuda, Manami Sasaki, Yasunobu Uchiyama, Naomi Tsuji, Benson Guest. 2019-04-13. High-Resolution X-ray Imaging Studies of Neutron Stars, Pulsar Wind Nebulae and Supernova Remnants. https://arxiv.org/abs/1904.06600

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