Could a slow stable hybrid star explain the central compact object in HESS J1731-347?-Reference-Cited by-同舟云学术

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Could a slow stable hybrid star explain the central compact object in HESS J1731-347?

Published:2024-08-19 Issue:4 Volume:110 Page:
ISSN:2470-0010
Container-title:Physical Review D
language:en
Short-container-title:Phys. Rev. D

Author:

Mariani Mauro¹²^ORCID,Ranea-Sandoval Ignacio F.¹²^ORCID,Lugones Germán³^ORCID,Orsaria Milva G.¹²^ORCID

Affiliation:

1. Universidad Nacional de La Plata

2. CONICET

3. Universidade Federal do ABC

Funder

Universidad Nacional de La Plata

Consejo Nacional de Investigaciones Científicas y Técnicas

National Science Foundation

Conselho Nacional de Desenvolvimento Científico e Tecnológico

Fundação de Amparo à Pesquisa do Estado de São Paulo

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.110.043026/fulltext

Reference73 articles.

1. PULSAR J0453+1559: A DOUBLE NEUTRON STAR SYSTEM WITH A LARGE MASS ASYMMETRY

2. Masses, Radii, and the Equation of State of Neutron Stars

3. J0453+1559: A Neutron Star–White Dwarf Binary from a Thermonuclear Electron-capture Supernova?

4. A strangely light neutron star within a supernova remnant

5. Do Central Compact Objects have Carbon Atmospheres?

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