154 citations · 584 across the 14 of their papers we have counts for
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Structure of the hot molecular core G10.47+0.03
Rainer Rolffs, Peter Schilke, Qizhou Zhang +1
The physical structure of hot molecular cores, where forming massive stars have heated up dense dust and gas, but have not yet ionized the molecules, poses a prominent challenge in…
Submillimeter continuum observations of Sagittarius B2 at subarcsecond spatial resolution
S. -L. Qin, P. Schilke, R. Rolffs +3
We report the first high spatial resolution submillimeter continuum observations of the Sagittarius B2 cloud complex using the Submillimeter Array (SMA). With the subarcsecond reso…
Hot HCN around young massive stars at 0.1" resolution
Rainer Rolffs, Peter Schilke, Friedrich Wyrowski +4
Massive stars form deeply embedded in dense molecular gas, which they stir and heat up and ionize. During an early phase, the ionization is confined to hypercompact HII regions, an…