Figure 1 from PLANETARY SYSTEM FORMATION IN THE PROTOPLANETARY DISK AROUND HL TAURI

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PLANETARY SYSTEM FORMATION IN THE PROTOPLANETARY DISK AROUND HL TAURI

Authors: Eiji Akiyama, Yasuhiro Hasegawa, Masahiko Hayashi, and Satoru Iguchi

2016 The Astrophysical Journal 818 158.

Provider: AAS Journals

Caption: Figure 1.

Dust continuum emission maps of HL Tau at 2.9 mm (a), 1.3 mm (b), and 0.87 mm (c) are provided with corresponding images of their synthesized beam maps (psf) and uv-coverages. The beam size at each wavelength is provided as a white filled ellipse in the lower left corner in the top panels.

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