Formation of long-period post-common-envelope binaries: II. Explaining the self-lensing binary KOI 3278

Publication:
Formation of long-period post-common-envelope binaries: II. Explaining the self-lensing binary KOI 3278

cris.virtual.department	Departamento de Física
cris.virtual.orcid	0000-0003-3903-8009
cris.virtualsource.department	753137e1-cbf8-4c58-8957-4305146fa79b
cris.virtualsource.orcid	753137e1-cbf8-4c58-8957-4305146fa79b
dc.contributor.author	Schreiber, Matthias
dc.contributor.author	Belloni, D.
dc.date.accessioned	2026-10-07T17:39:14Z
dc.date.available	2026-10-07T17:39:14Z
dc.date.issued	2024-06
dc.description.abstract	Context. The vast majority of close binaries containing a compact object, including the progenitors of supernovae Ia and at least a substantial fraction of all accreting black holes in the Galaxy, form through common-envelope (CE) evolution. Despite this
dc.identifier.doi	10.1051/0004-6361/202449320
dc.identifier.eissn	14320746
dc.identifier.issn	00046361
dc.identifier.uri	https://doi.org/10.1051/0004-6361/202449320
dc.identifier.uri	https://cris.usm.cl/handle/123456789/6174
dc.language.iso	en
dc.relation.journal	Astronomy and Astrophysics
dc.subject	Binaries: General
dc.subject	Methods: Numerical
dc.subject	Stars: Agb And Post-Agb
dc.subject	Stars: Evolution
dc.subject	Stars: Individual: Koi 3278
dc.subject	White Dwarfs
dc.title	Formation of long-period post-common-envelope binaries: II. Explaining the self-lensing binary KOI 3278
dc.type	Research Article
dspace.entity.type	Publication
oaire.citation.volume	687
oairecerif.author.affiliation	#PLACEHOLDER_PARENT_METADATA_VALUE#
oairecerif.author.affiliation	Departamento de Física