Figure 2 from Resolving the Polarized Dust Emission of the Disk around the Massive Star Powering the HH 80

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Resolving the Polarized Dust Emission of the Disk around the Massive Star Powering the HH 80–81 Radio Jet

Authors: J. M. Girart, M. Fernández-López, Z.-Y. Li, H. Yang, R. Estalella, G. Anglada, N. Áñez-López, G. Busquet, C. Carrasco-González, S. Curiel, R. Galvan-Madrid, J. F. Gómez, I. de Gregorio-Monsalvo, I. Jiménez-Serra, R. Krasnopolsky, J. Martí, M. Osorio, M. Padovani, R. Rao, L. F. Rodríguez, and J. M. Torrelles

2018 The Astrophysical Journal Letters 856 L27.

Provider: AAS Journals

Caption: Figure 2.

Radial profile of the 1.14 mm dust emission from the GGD27 MM1 disk, obtained by averaging the emission over elliptical rings (filled squares). The blue and dashed line show the best-fitted profile (see Section 3.1) and the beam profile, respectively. The error bars show the rms dispersion within each ring for the data. The vertical dotted line indicates R_turn, the radius where the power law changes.

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