Figure 4 from Resolving the Polarized Dust Emission of the Disk around the Massive Star Powering the HH 80

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

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 4.

Left panel: histogram of the distribution of the polarization position angles for the disk’s inner region (R < 0.″10). The dashed line indicates the position angle of the disk minor axis. Right panel: histogram of the differences between the polarization position angles and the disk azimuthal angles for the disk’s outer region (R > 0.″10).

Other Images in This Article

Copyright and Terms & Conditions