activity
20172022
most citedProperties of Hi-GAL clumps in the inner Galaxy]{The Hi-GAL compact source catalogue. I. The physical properties of the clumps in the inner Galaxy ()

201 citations · 245 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.GA202219 cited

CHEMOUT: CHEMical complexity in star-forming regions of the OUTer Galaxy. I. Organic molecules and tracers of star-formation activity

F. Fontani, L. Colzi, L. Bizzocchi +8

The outer Galaxy is an environment with metallicity lower than the Solar one. Because of this, the formation and survival of molecules in star-forming regions located in the inner…

astro-ph.GA202217 cited

The sharp ALMA view of infall and outflow in the massive protocluster G31.41+0.31

M. T. Beltrán, V. M. Rivilla, R. Cesaroni +15

Context. To better understand the formation of high-mass stars, it is fundamental to investigate how matter accretes onto young massive stars, how it is ejected, and how all this d…

astro-ph.GA20206 cited

Disks around O-type young stellar objects

Maite Beltrán

Accretion disks are one of the key ingredients of the star formation process. They redistribute angular momentum and, in the case of high-mass stars (M > 8Msun), disks would reliev…

astro-ph.IM20192 cited

Wide Bandwidth Considerations for ALMA Band 2

Tony Mroczkowski, Carlos De Breuck, Ciska Kemper +9

One of the main considerations in the ALMA Development Roadmap for the future of operations beyond 2030 is to at least double its on-sky instantaneous bandwidth capabilities. Thank…

astro-ph.GA2018

Resolving the Structure and Kinematics of the Youngest HII Regions and Radio Jets from Young Stellar Objects

Roberto Galván-Madrid, Maite Beltrán, Adam Ginsburg +4

In this contribution we explore the new science that a Next Generation Very Large Array (ngVLA) would be able to perform on the topics of the youngest HII regions and (proto)stella…

astro-ph.GA2017201 cited

Properties of Hi-GAL clumps in the inner Galaxy]{The Hi-GAL compact source catalogue. I. The physical properties of the clumps in the inner Galaxy ()

D. Elia, S. Molinari, E. Schisano +83

Hi-GAL is a large-scale survey of the Galactic plane, performed with Herschel in five infrared continuum bands between 70 and 500 m. We present a band-merged catalogue of spatia…