273 citations · 2k across the 34 of their papers we have counts for
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Spectral Hardening of Large Solar Flares
Paolo C. Grigis, Arnold O. Benz
RHESSI observations are used to quantitatively study the hard X-ray evolution in 5 large solar flares selected for spectral hardening in the course of the event. The X-ray bremsstr…
Tracing high energy radiation with molecular lines near deeply embedded protostars
P. Stauber, A. O. Benz, J. K. Jorgensen +3
Submillimeter lines of CN, NO, CO+ and SO+, and upper limits on SH+ and N2O are observed with the James Clerk Maxwell Telescope in two high-mass and up to nine low-mass young stell…
Water destruction by X-rays in young stellar objects
P. Stauber, J. K. Jorgensen, E. F. van Dishoeck +2
We study the H2O chemistry in star-forming environments under the influence of a central X-ray source and a central far ultraviolet (FUV) radiation field. The gas-phase water chemi…
X-ray chemistry in envelopes around young stellar objects
P. Staeuber, S. D. Doty, E. F. van Dishoeck +1
We present chemical models of the envelope of a young stellar object (YSO) exposed to a central X-ray source. The models are applied to the massive star-forming region AFGL 2591 fo…
X-ray Chemistry in the Envelopes around Young Stellar Objects
P. Staeuber, A. O. Benz, S. D. Doty +1
We have studied the influence of X-rays from a massive young stellar object (YSO) on the chemistry of its own envelope by extending the models of Doty et al. (2002) and Staeuber et…
Influence of UV radiation from a massive YSO on the chemistry of its envelope
P. Stauber, S. D. Doty, E. F. van Dishoeck +2
We have studied the influence of far ultraviolet (UV) radiation from a massive young stellar object (YSO) on the chemistry of its own envelope by extending the models of Doty et al…