Formation of long-period post-common envelope binaries: I. No extra energy is needed to explain oxygen-neon white dwarfs paired with AFGK-type main-sequence stars

被引：0

作者：

Belloni, Diogo ^{[1
]}

Zorotovic, Monica ^{[2
]}

Schreiber, Matthias R. ^{[1
,3
]}

Parsons, Steven G. ^{[4
]}

Moe, Maxwell ^{[5
]}

Garbutt, James A. ^{[4
]}

机构：

[1] Departamento de Física, Universidad Técnica Federico Santa María, Av. España 1680, Valparaíso, Chile

[2] Instituto de Física y Astronomía, Universidad de Valparaíso, Av. Gran Bretaña 1111, Valparaíso, Chile

[3] Millenium Nucleus for Planet Formation, Valparaíso, Chile

[4] Department of Physics and Astronomy, University of Sheffield, Sheffield,S3 7RH, United Kingdom

[5] Department of Physics & Astronomy, University of Wyoming, Laramie,WY 82071, United States

来源：

Astronomy and Astrophysics | 2024年 / 686卷

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