MXB 1658-298
작성자: SevenSpheres Cham Vision
출시일:
MXB 1658-298, also known as V2134 Ophiuchi, is a distant X-ray binary star system consisting of a pulsar and a K-type main sequence star about 32,615 light-years away in the constellation Ophiuchus. In 2017, a massive substellar companion about 23 times the mass of Jupiter was detected via eclipse timing variations, completing a single orbit around both stars once every 2.1 years
이 페이지의 번역에 여기에서 도움을 주세요.
애드온을 설치하는 방법은? 여기에서 확인하세요.