Accretion‐induced collapse to third family compact stars as trigger for eccentric orbits of millisecond pulsars in binaries-Reference-Cited by-同舟云学术

Accretion‐induced collapse to third family compact stars as trigger for eccentric orbits of millisecond pulsars in binaries

Published:2019-11 Issue:9-10 Volume:340 Page:878-884
ISSN:0004-6337
Container-title:Astronomische Nachrichten
language:en
Short-container-title:Astron. Nachr

Author:

Alvarez‐Castillo David Edwin¹,Antoniadis John²,Ayriyan Alexander³⁴,Blaschke David¹⁵⁶,Danchev Victor⁷,Grigorian Hovik³⁴⁸,Largani Noshad Khosravi⁵,Weber Fridolin⁹¹⁰

Affiliation:

1. Bogoliubov Laboratory for Theoretical Physics Joint Institute for Nuclear Research Dubna Russia

2. Max‐Planck‐Institut für Radioastronomie and Argelander Institut für Astronomie Bonn Germany

3. Laboratory for Information Technologies Joint Institute for Nuclear Research Dubna Russia

4. Computational Physics and IT Division A.I. Alikhanyan National Science Laboratory Yerevan Armenia

5. Institute of Theoretical Physics University of Wroclaw Wroclaw Poland

6. National Research Nuclear University (MEPhI) Moscow Russia

7. Department of Physics Sofia University Sofia Bulgaria

8. Department of Physics Yerevan State University Yerevan Armenia

9. Department of Physics San Diego State University San Diego California

10. Department of Physics University of California San Diego California

Funder

National Science Foundation

Russian Science Foundation

Publisher

Wiley

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1002/asna.201913752

Reference42 articles.

1. GW170817: Measurements of Neutron Star Radii and Equation of State

2. Compact Stars with Sequential QCD Phase Transitions

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