Characterizing young protostellar disks with the CALYPSO IRAM-PdBI survey: large Class 0 disks are rare

A. J. Maury; Ph. André; L. Testi; S. Maret; A. Belloche; P. Hennebelle; S. Cabrit; C. Codella; F. Gueth; L. Podio; S. Anderl; A. Bacmann; S. Bontemps; M. Gaudel; B. Ladjelate; C. Lefèvre; B. Tabone; B. Lefloch

doi:10.1051/0004-6361/201833537

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Volume 621 (January 2019)

A&A, 621 (2019) A76

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Fig. C.16

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Same as Fig. C.16 for L1157. The red Plummer + Gaussian (PG) model that includes an unresolved Gaussian component (see Table 6 for moreinformations on both models) is statistically better than the black Plummer-only (Pl) model at 231 GHz. At 94 GHz, the best-fit model is the Plummer-envelope model.

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