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Testing grain-surface chemistry in massive hot-core regions

Astronomy and astrophysics (Berlin), 2007-04, Vol.465 (3), p.913-929

2007

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Desorption rates and sticking coefficients for CO and N2 interstellar ices

Astronomy and astrophysics (Berlin), 2006-04, Vol.449 (3), p.1297-1309

2006

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

Astronomy and astrophysics (Berlin), 2008-09, Vol.488 (3), p.959-968

2008

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Probing the effects of external irradiation on low-mass protostars through unbiased line surveys

Astronomy and astrophysics (Berlin), 2015-12, Vol.584, p.A28

2015

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H-atom bombardment of CO2, HCOOH, and CH3CHO containing ices

Astronomy and astrophysics (Berlin), 2007-11, Vol.474 (3), p.1061-1071

2007

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

Astronomy and astrophysics (Berlin), 2007-02, Vol.462 (3), p.1187-1198

2007

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Structure of evolved cluster-forming regions

Astronomy and astrophysics (Berlin), 2011-03, Vol.527, p.A68

2011

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Observations of nitrogen isotope fractionation in deeply embedded protostars

Astronomy and astrophysics (Berlin), 2014-12, Vol.572, p.1-16

2014

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Hydrogenation reactions in interstellar CO ice analogues: A combined experimental/theoretical approach

Astronomy and astrophysics (Berlin), 2009-10, Vol.505 (2), p.629-639

2009

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Infrared spectroscopy of HCOOH in interstellar ice analogues

Astronomy and astrophysics (Berlin), 2007-08, Vol.470 (2), p.749-759

2007

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

The Astrophysical journal, 2008-05, Vol.678, p.985

2008

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Competition between CO and N2 Desorption from Interstellar Ices

The Astrophysical journal, 2005-03, Vol.621 (1), p.L33-L36

2005

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Desorption rates and sticking coefficients for CO and N 2 interstellar ices

Astronomy and astrophysics (Berlin), 2006-04, Vol.449 (3), p.1297-1309

2006

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Competition between CO and N 2 Desorption from Interstellar Ices

The Astrophysical journal, 2005-03, Vol.621 (1), p.L33-L36

2005

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Hydrogenation reactions in interstellar CO ice analogues

Astronomy and astrophysics (Berlin), 2009-10, Vol.505 (2), p.629-639

2009

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Formation of alcohols on ice surfaces

Proceedings of the International Astronomical Union, 2008-02, Vol.4 (S251), p.377-382

2008

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Dimethyl ether in its ground state, v = 0, and lowest two torsionally excited states, v 11 = 1 and v 15 = 1, in the high-mass star-forming region G327.3-0.6

Astronomy and astrophysics (Berlin), 2013-04, Vol.552, p.A122

2013

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A $\mathsf{3{-}5~\mu}$m VLT spectroscopic survey of embedded young low mass stars I

Astronomy and astrophysics (Berlin), 2003-09, Vol.408 (3), p.981-1007

2003

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Laboratory rotational spectra of the dimethyl ether 13 C-isotopologues up to 1.5 THz

Astronomy and astrophysics (Berlin), 2013-10, Vol.558, p.A112

2013

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Laboratory rotational spectra of the dimethyl ether super(13)C-isotopologues up to 1.5 THz

Astronomy and astrophysics (Berlin), 2013-10, Vol.558, p.np-np

2013

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Laboratory rotational spectra of the dimethyl ether 13C-isotopologues up to 1.5 THz

Astronomy and astrophysics (Berlin), 2013-10, Vol.558

2013

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Spectroscopy and Processing of Interstellar Ice Analogs

Astrochemistry: From Laboratory Studies to Astronomical Observations (AIP Conference Proceedings Volume 855), 2006, Vol.855, p.113-121

2006

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Dimethyl ether in its ground state, v = 0, and lowest two torsionally excited states, v sub(11) = 1 and v sub(15) = 1, in the high-mass star-forming region G327.3-0.6

Astronomy and astrophysics (Berlin), 2013-04, Vol.552, p.np-np

2013

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Dimethyl ether in its ground state, v = 0, and lowest two torsionally excited states, v11 = 1 and v15 = 1, in the high-mass star-forming region G327.3-0.6

Astronomy and astrophysics (Berlin), 2013-04, Vol.552

2013

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H-atom bombardment of CO 2 , HCOOH, and CH 3 CHO containing ices

Astronomy and astrophysics (Berlin), 2007-11, Vol.474 (3), p.1061-1071

2007

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Testing grain-surface chemistry in massive hot-core regions

Desorption rates and sticking coefficients for CO and N2 interstellar ices

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

Probing the effects of external irradiation on low-mass protostars through unbiased line surveys

H-atom bombardment of CO2, HCOOH, and CH3CHO containing ices

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

Structure of evolved cluster-forming regions

Observations of nitrogen isotope fractionation in deeply embedded protostars

Hydrogenation reactions in interstellar CO ice analogues: A combined experimental/theoretical approach

Infrared spectroscopy of HCOOH in interstellar ice analogues

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

Competition between CO and N2 Desorption from Interstellar Ices

Desorption rates and sticking coefficients for CO and N 2 interstellar ices

Competition between CO and N 2 Desorption from Interstellar Ices

Hydrogenation reactions in interstellar CO ice analogues

Formation of alcohols on ice surfaces

Dimethyl ether in its ground state, v = 0, and lowest two torsionally excited states, v 11 = 1 and v 15 = 1, in the high-mass star-forming region G327.3-0.6

A $\mathsf{3{-}5~\mu}$m VLT spectroscopic survey of embedded young low mass stars I

Laboratory rotational spectra of the dimethyl ether 13 C-isotopologues up to 1.5 THz

Laboratory rotational spectra of the dimethyl ether super(13)C-isotopologues up to 1.5 THz

Laboratory rotational spectra of the dimethyl ether 13C-isotopologues up to 1.5 THz

Spectroscopy and Processing of Interstellar Ice Analogs

Dimethyl ether in its ground state, v = 0, and lowest two torsionally excited states, v sub(11) = 1 and v sub(15) = 1, in the high-mass star-forming region G327.3-0.6

Dimethyl ether in its ground state, v = 0, and lowest two torsionally excited states, v11 = 1 and v15 = 1, in the high-mass star-forming region G327.3-0.6

H-atom bombardment of CO 2 , HCOOH, and CH 3 CHO containing ices

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