Ring Surface Density
Ring Surface Density is a physical quantity that represents the mass per unit area of a planetary ring, distinguishing it from volume-based densities by characterizing the distribution of ring material in two-dimensional projection perpendicular to the orbital plane.
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167
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99
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2017–2026
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ALMA continuum observations of the protoplanetary disk AS 209
D. Fedele, Marco Tazzari, Richard A Booth et al. · Astronomy and Astrophysics · 2017 · 176 citations · Full text
Natural Sciences, Astronomy, Physics +14
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Max Planck Institute for Astronomy
Heidelberg, Germany
5 h-index
7 publications
871 citations
Max Planck Institute for Extraterrestrial Physics
Garching bei München, Germany
5 h-index
6 publications
779 citations
California Institute of Technology
Pasadena, United States
4 h-index
9 publications
480 citations
Jet Propulsion Laboratory
Pasadena, United States
4 h-index
9 publications
288 citations
Arcetri Astrophysical Observatory
Florence, Italy
4 h-index
8 publications
663 citations
University of Cambridge
Cambridge, United Kingdom
4 h-index
10 publications
835 citations
European Southern Observatory
Garching bei München, Germany
4 h-index
6 publications
304 citations

Atacama Large Millimeter Submillimeter Array
Santiago, Chile
3 h-index
7 publications
2.2K citations
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ApJ · 8 publications · 752 citations
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JGR · 4 publications · 228 citations
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4 publications · 61 citations
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4 publications · 488 citations
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AJ · 3 publications · 65 citations
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