activity
20172026
most citedThe Green Bank Ammonia Survey (GAS): First Results of NH3 mapping the Gould Belt

159 citations · 926 across the 24 of their papers we have counts for

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Showing 2021Show all

5 papers · 1 filter

astro-ph.GA2021★ 44 cited

The cosmic-ray ionisation rate in the pre-stellar core L1544

Elena Redaelli, Olli Sipilä, Marco Padovani +3

Context. Cosmic rays (CRs) play an important role in the chemistry and dynamics of the interstellar medium. In dense environments, they represent the main ionising agent, driving t…

astro-ph.GA2021★ 25 cited

Are massive dense clumps truly sub-virial? A new analysis using Gould Belt ammonia data

Ayushi Singh, Christopher D. Matzner, Rachel K. Friesen +21

Dynamical studies of dense structures within molecular clouds often conclude that the most massive clumps contain too little kinetic energy for virial equilibrium, unless they are…

astro-ph.GA2021★ 15 cited

First survey of HCNH in high-mass star-forming cloud cores

F. Fontani, L. Colzi, E. Redaelli +2

Most stars in the Galaxy, including the Sun, were born in high-mass star-forming regions. It is hence important to study the chemical processes in these regions to better understan…

astro-ph.GA2021★ 34 cited

Identification of prestellar cores in high-mass star forming clumps via observations with ALMA

E. Redaelli, S. Bovino, A. Giannetti +5

Context. The different theoretical models concerning the formation of high-mass stars make distinct predictions regarding their progenitors, i.e. the high-mass prestellar cores. Ho…

astro-ph.GA2021★ 25 cited

Transition from Coherent Cores to Surrounding Cloud in L1688

Spandan Choudhury, Jaime E. Pineda, Paola Caselli +8

Stars form in cold dense cores showing subsonic velocity dispersions. The parental molecular clouds display higher temperatures and supersonic velocity dispersions. The transition…