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Substructure Formation in a Protostellar Disk of L1527 IRS

  • Authors: Riouhei Nakatani, Hauyu Baobab Liu, Satoshi Ohashi, Yichen Zhang, Tomoyuki Hanawa, Claire Chandler, Yoko Oya, and Nami Sakai

2020 The Astrophysical Journal Letters 895 L2.

  • Provider: AAS Journals

Caption: Figure C2.

Examples of our synthetic observations. (Left) model emission of a smooth disk with Σ0 = 104 g cm−2 and i = 10 deg. The corresponding flux density is ≈4.9 mJy. (middle) observed image with VLA B-configuration and integration time of an hour. Recovered flux density is ≈4.3 mJy (right) observed image with VLA A-configuration and integration time of two hours. Recovered flux density is ≈0.84 mJy.

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