activity
20052020
most citedProbing the initial conditions of high-mass star formation. II. Fragmentation, stability, and chemistry

163 citations · 243 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2020★ 11 cited

Probing the initial conditions of high-mass star formation -- IV. Gas dynamics and NHD chemistry in high-mass precluster and protocluster clumps

Chuan-Peng Zhang, Guang-Xing Li, Thushara Pillai +4

The initial stage of star formation is a complex area study because of its high density and low temperature. Under such conditions, many molecules become depleted from the gas phas…

astro-ph.GA2019★ 9 cited

Probing the initial conditions of high-mass star formation. III. Fragmentation and triggered star formation

Chuan-Peng Zhang, Timea Csengeri, Friedrich Wyrowski +6

Massive clumps tend to fragment into clusters of cores and condensations, some of which form high-mass stars. In this work, we study the structure of massive clumps at different sc…

astro-ph.GA2011★ 163 cited

Probing the initial conditions of high-mass star formation. II. Fragmentation, stability, and chemistry

T. Pillai, J. Kauffmann, F. Wyrowski +3

We present a new high-resolution study of pre-protocluster regions in tracers exclusively probing the coldest and dense gas (NH_2D). The data are used to constrain the chemical, th…

astro-ph2007

Star formation in Perseus: III. Outflows

J. Hatchell, G. A. Fuller, J. S. Richer

We present a search for outflows towards 51 submillimetre cores in Perseus. With consistently derived outflow properties from a large homogeneous dataset within one molecular cloud…

astro-ph2006★ 27 cited

The JCMT Spectral Legacy Survey

R. Plume, G. A. Fuller, F. Helmich +30

Stars form in the densest, coldest, most quiescent regions of molecular clouds. Molecules provide the only probes which can reveal the dynamics, physics, chemistry and evolution of…

astro-ph2005★ 13 cited

An observational survey of molecular emission ahead of Herbig-Haro objects

S. Viti, J. M. Girart, J. Hatchell

Context. A molecular survey recently performed ahead of HH~2 supports the idea that the observed molecular enhancement is due to UV radiation from the HH object. Aims. The aim of t…