Skip to main content
. Author manuscript; available in PMC: 2016 Sep 14.
Published in final edited form as: Astrophys J. 2014 Nov 4;796(1):41. doi: 10.1088/0004-637X/796/1/41

Fig. 17.

Fig. 17

Top Panel: Comparison between predicted detected meteor rates assuming ZoDy to be the incoming flux and those observed by Arecibo. Bottom Panel: Comparison between predicted radial velocities of detected meteors assuming ZoDy to be the incoming flux and those observed by Arecibo.