A computer program for fast non-LTE analysis of interstellar line spectra - With diagnostic plots to interpret observed line intensity ratios
A&A, 468 2 (2007) 627-635
Published online: 2007-04-03
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Possible planet formation in the young, low-mass, multiple stellar system GG Tau A
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Evidence for large grains in the star-forming filament OMC 2/3
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H2CO and H110α observations towards NH3 sources
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Champagne flutes and brandy snifters: modelling protostellar outflow–cloud chemical interfaces
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