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Asymmetry and Variability in the HH 30 Circumstellar Disk

  • Authors: Alan M. Watson and Karl R. Stapelfeldt

Watson & Stapelfeldt 2007 The Astronomical Journal 133 845.

  • Provider: AAS Journals

Caption: Fig. 9.

Vertical brightness profiles of the right (solid line) and left (dotted line) sides of the (a) 2000 February F675W image (with the right side brighter) and (b) 2001 February F675W image (with the left side brighter). The dashed line shows the difference. The flux units are arbitrary.

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