4U 1556–60 as a very faint neutron star X-ray binary at 700 pc with an undetected radio jet

Context. 4U 1556–60 is a low-mass X-ray binary that was discovered more than 50 years ago as a persistent X-ray source; however, very little was known about it. Recently, Gaia obtained a parallax for the optical counterpart that places 4U 1556–60 at a distance of only about 700 pc, making it one of...

Полное описание

Библиографические подробности

Главные авторы:	Pattie E. C., Maccarone T. J., Russell T., Bachetti M., Degenaar N., Kupfer T.
Формат:	Artigo
Язык:	Inglês
Опубликовано:	EDP Sciences 2026-03-01
Серии:	Astronomy & Astrophysics
Предметы:	accretion accretion disks binaries: general stars: jets stars: neutron x-rays: binaries
Online-ссылка:	https://www.aanda.org/articles/aa/full_html/2026/03/aa57591-25/aa57591-25.html
Метки:	Добавить метку Нет меток, Требуется 1-ая метка записи!