BW Sculptoris
id:
bw-sculptoris-173-3207302
title:
BW Sculptoris
text:
BW Sculptoris is WZ Sge-type dwarf nova and a candidate period bouncer. The binary consists of a white dwarf and a brown dwarf donor that orbits the white dwarf every 78.23 minutes. BW Sculptoris is one of the closest and brightest cataclysmic variable stars with a brightness of magnitude16.5 and a distance of 93.3 parsecs. It also has the shortest period for any CVs known to date. BW Sculptoris was discovered in 1997 by two teams. Abbott et al. discovered it with ROSAT as RX J2353.0-3852. Augus
brand slug:
wiki
category slug:
encyclopedia
description:
Dwarf nova in the constellation Sculptor
original url:
https://en.wikipedia.org/wiki/BW_Sculptoris
date created:
2024-01-16T17:15:12Z
date modified:
2024-09-02T01:48:13Z
main entity:
{"identifier":"Q9163616","url":"https://www.wikidata.org/entity/Q9163616"}
image:
{"content_url":"https://upload.wikimedia.org/wikipedia/commons/b/b0/BW_Sculptoris.jpg","width":500,"height":500}
fields total:
13
integrity:
16