HD 101584
id:
hd-101584-197-11490220
title:
HD 101584
text:
HD 101584 is a suspected post-common envelope binary about 1,800 to 5,900 light-years distant in the constellation of Centaurus. The system is bright at optical wavelengths with an apparent visual magnitude of about 7. The primary is either a post-AGB star, but more likely a post-RGB star. The secondary is a red dwarf or possibly a low-luminosity white dwarf, which orbits the primary every 150-200 days. The system is surrounded by a slowly rotating circumbinary disk, probably with a face-on orie
brand slug:
wiki
category slug:
encyclopedia
description:
Star in the constellation Centaurus
original url:
https://en.wikipedia.org/wiki/HD_101584
date created:
date modified:
2024-01-20T05:23:09Z
main entity:
{"identifier":"Q66621664","url":"https://www.wikidata.org/entity/Q66621664"}
image:
{"content_url":"https://upload.wikimedia.org/wikipedia/commons/3/37/HD_101584.jpg","width":2048,"height":1536}
fields total:
13
integrity:
15