activity
20182023
most citedModeling the accretion disk around the high-mass protostar GGD 27-MM1

30 citations · 93 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2023

Radio survey of the stellar population in the infrared dark cloud G14.225-0.506

Elena Díaz-Márquez, Roger Grau, Gemma Busquet +8

The IRDC G14.225-0.506 is associated with a network of filaments, which result in two different dense hubs, as well as with several signposts of star formation activity. The aim of…

astro-ph.GA202029 cited

The role of the magnetic field in the fragmentation process: the case of G14.225-0.506

N. Añez-López, G. Busquet, P. M. Koch +8

B-fields are predicted to play a role in the formation of filamentary structures and their fragmentation process. We aim at investigating the role of the B-field in the process of…

astro-ph.SR202011 cited

Characterizing the radio continuum nature of sources in the massive star-forming region W75N (B)

A. Rodríguez-Kamenetzky, C. Carrasco-González, J. M. Torrelles +11

The massive star-forming region W75N~(B) is thought to host a cluster of massive protostars (VLA~1, VLA~2, and VLA~3) undergoing different evolutionary stages. In this work, we pre…

astro-ph.SR201930 cited

Modeling the accretion disk around the high-mass protostar GGD 27-MM1

N. Añez-Lopez, M. Osorio, G. Busquet +9

Recent high-angular resolution (40 mas) ALMA observations at 1.14 mm resolve a compact (R~200 au) flattened dust structure perpendicular to the HH 80-81 jet emanating from the GGD…

astro-ph.SR201923 cited

Unveiling a cluster of protostellar disks around the massive protostar GGD27 MM1

G. Busquet, J. M. Girart, R. Estalella +9

We used ALMA to observe the star-forming region GGD27 at 1.14 mm with an unprecedented angular resolution, 40 mas (56 au) and sensitivity (0.002 Msun). We detected a cluster of 25…

astro-ph.SR2018

Resolving the polarized dust emission of the disk around the massive star powering the HH~80-81 radio jet

J. M. Girart, M. Fernandez-Lopez, Z. -Y. Li +18

Here we present deep (16 mumJy), very high (40 mas) angular resolution 1.14 mm, polarimetric, Atacama Large Millimeter/submillimeter Array (ALMA) observations towards the massive p…