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...y. They have been observed in the Milky Way's halo and within other nearby galaxies. ...SMC, respectively) which produce a well-known complex of HVCs called the [[Magellanic Stream]]. Because of the various possible mechanisms that could potentially ...

...The OGLE-III Catalog of Variable Stars. I. Classical Cepheids in the Large Magellanic Cloud |author1=Soszynski, I. |author2=Poleski, R. |author3=Udalski, A. |aut ...ckering |first2=Edward C. |title=Periods of 25 Variable Stars in the Small Magellanic Cloud |journal=Harvard College Observatory Circular |date=1912 |volume=173 ...

...en used to clarify many characteristics of our galaxy, such as the local [[spiral arm]] structure and the Sun's distance from the [[galactic plane]].<ref nam ...more are known in the [[Magellanic Clouds]], with more discovered in other galaxies;<ref>{{cite journal|bibcode=2003ASPC..298..237S|title=Cepheids: Observation ...

...y|satellites]] as well as the internal kinematics of more distant [[Galaxy|galaxies]]. Measurement of the kinematics of stars in different subcomponents of the ...the influence of [[gravity]]. Stellar-dynamical models of systems such as galaxies or star clusters are often compared with or tested against stellar-kinemati ...

...}}</ref> for a [[gravitational wave]] emanating from the [[inspiral|inward spiral]] and [[Stellar collision|merger]] of [[Binary black hole|two black holes]] ...es from a system of two objects in mutual orbit would cause them to slowly spiral inwards, although again, this effect would be extremely minute and thus cha ...

...ame="AJL-20200601">{{cite journal |author=Bhandan, Shivani |title=The Host Galaxies and Progenitors of Fast Radio Bursts Localized with the Australian Square K ...ft; and FRB 190608, at bottom right.<ref>{{cite web|title=Fast Radio Burst Galaxies|url=https://esahubble.org/images/opo2110a/|website=ESA/Hubble|date=20 May 2 ...