Figure 1 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 1.

Image of the GGD27 MM1 disk in units of brightness temperature. (a) Original map; (b) map obtained after subtracting the compact source from the visibilities. The color scale is the same for the two panels. The black contours are 5, 10, 20, 50, 100, and 200 K, and the white contours 400 and 600 K. The synthesized beam is shown in the right-bottom corner of the bottom panel.

Other Images in This Article

Copyright and Terms & Conditions