Image Details
Caption: Figure 4.
Surface brightness profiles of dust tails that are normalized to the brightness of the nucleus from 2013 September to December. The dust tail (Tail I) observed on 2014 February 11 is not considered due to its low S/N. The upper and lower horizontal axes show the radial distance from the nucleus in units of the radiation pressure parameter β and arcseconds, respectively.
© 2023. The Author(s). Published by the American Astronomical Society.