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20032026
most citedThe c2d Spitzer Spectroscopic Survey of Ices Around Low-Mass Young Stellar Objects: I. H2O and the 5-8 um Bands

384 citations · 2.6k across the 22 of their papers we have counts for

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astro-ph2008★ 148 cited

An interferometric study of the low-mass protostar IRAS 16293-2422: small scale organic chemistry

S. E. Bisschop, J. K. Jorgensen, T. L. Bourke +2

Aims: To investigate the chemical relations between complex organics based on their spatial distributions and excitation conditions in the low-mass young stellar objects IRAS 16293…

astro-ph2008★ 194 cited

The c2d Spitzer spectroscopy survey of ices around low-mass young stellar objects, III: CH4

Karin I. Oberg, A. C. Adwin Boogert, Klaus M. Pontoppidan +4

CH4 is proposed to be the starting point of a rich organic chemistry. Solid CH4 abundances have previously been determined mostly toward high mass star forming regions. Spitzer/IRS…

astro-ph2008★ 384 cited

The c2d Spitzer Spectroscopic Survey of Ices Around Low-Mass Young Stellar Objects: I. H2O and the 5-8 um Bands

A. Boogert, K. Pontoppidan, C. Knez +23

With the goal to study the physical and chemical evolution of ices in solar-mass systems, a spectral survey is conducted of a sample of 41 low luminosity YSOs using 3-38 um Spitzer…

astro-ph2007★ 59 cited

Infrared spectroscopy of HCOOH in interstellar ice analogues

S. E. Bisschop, G. W. Fuchs, A. C. A. Boogert +2

Context: HCOOH is one of the more common species in interstellar ices with abundances of 1-5% with respect to solid H2O. Aims: This study aims at characterizing the HCOOH spectral…

astro-ph2007★ 350 cited

Testing grain-surface chemistry in massive hot-core regions

S. E. Bisschop, J. K. Jorgensen, E. F. van Dishoeck +1

A partial submillimeter line-survey was performed toward 7 high-mass young stellar objects (YSOs) aimed at detecting H2CO, CH3OH, CH2CO, CH3CHO, C2H5OH, HCOOH, HNCO and NH2CHO. In…

astro-ph2006★ 102 cited

Effects of CO2 on H2O band profiles and band strengths in mixed H2O:CO2 ices

Karin I. Oberg, Helen J. Fraser, A. C. Adwin Boogert +4

H2O is the most abundant component of astrophysical ices. In most lines of sight it is not possible to fit both the H2O 3 um stretching, the 6 um bending and the 13 um libration ba…