NGC 1023

Hydrogen bridge

← Previous revision Revision as of 00:44, 29 April 2026 Line 55: Line 55: | volume=332 | issue=1 | pages=65–77 | date=May 2002 | volume=332 | issue=1 | pages=65–77 | date=May 2002 | doi=10.1046/j.1365-8711.2002.05269.x | doi=10.1046/j.1365-8711.2002.05269.x | arxiv=astro-ph/0112288 | bibcode=2002MNRAS.332...65D }}</ref> NGC 1023 has a [[satellite galaxy]] named NGC 1023A, which is a [[Magellanic spiral]] galaxy; its globular cluster system is much smaller, estimated to be around six individuals.<ref name=Young/> | arxiv=astro-ph/0112288 | bibcode=2002MNRAS.332...65D }}</ref> NGC 1023 has a [[satellite galaxy]] named NGC 1023A, which is a [[Magellanic spiral]] galaxy; its globular cluster system is much smaller, estimated to be around six individuals.<ref name=Young/> A bridge of neutral hydrogen extends from NGC 1023 to NGC 1023A, which may indicate a possible interaction.<ref>{{cite journal | title=Is NGC 1023/1023A an interacting system ? | last1=Capaccioli | first1=M. | display-authors=etal | journal=Astronomy and Astrophysics | volume=169 | pages=54–62 | date=November 1986 | bibcode=1986A&A...169...54C }}</ref>

== References == == References ==