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Chains of dense cores in the Taurus L1495/B213 complex

Astronomy and astrophysics (Berlin), 2015-02, Vol.574, p.A104

2015

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CONSTRAINING THE ABUNDANCES OF COMPLEX ORGANICS IN THE INNER REGIONS OF SOLAR-TYPE PROTOSTARS

The Astrophysical journal, 2015-05, Vol.804 (2), p.1-30

2015

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The Case of H2C3O Isomers, Revisited: Solving the Mystery of the Missing Propadienone

The Astrophysical journal, 2019-06, Vol.878 (2)

2019

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Hydrodynamics with gas–grain chemistry and radiative transfer: comparing dynamical and static models

Astronomy and astrophysics (Berlin), 2018-07, Vol.615, p.A15

2018

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Dust Destruction in Nonradiative Shocks

The Astrophysical journal, 2019-09, Vol.882 (2), p.135

2019

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Is the Gas-phase OH+H2CO Reaction a Source of HCO in Interstellar Cold Dark Clouds? A Kinetic, Dynamic, and Modeling Study

The Astrophysical journal, 2017-11, Vol.850 (1)

2017

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Galactic Chemical Evolution of Radioactive Isotopes

The Astrophysical journal, , Vol.878 (2), p.156

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Water deuterium fractionation in the high-mass star-forming region G34.26+0.15 based on Herschel/HIFI data

Monthly notices of the Royal Astronomical Society, 2014-12, Vol.445 (2), p.1299-1299

2014

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Spitzer Observations of HH 54 and HH 7-11: Mapping the H2 Ortho-to-Para Ratio in Shocked Molecular Gas

The Astrophysical journal, 2006-10, Vol.649, p.816

2006

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Ortho-to-para ratio of NH2. Herschel-HIFI observations of ortho- and para-NH2 rotational transitions towards W31C, W49N, W51 and G34.3+0.1

Astronomy and astrophysics (Berlin), 2016-02, Vol.586, p.Art Nr. A128

2016

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Effect of the Surface Roughness of Icy Grains on Molecular Oxygen Chemistry in Molecular Clouds

The Astrophysical journal, 2019-09, Vol.882 (2), p.131

2019

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History of the solar-type protostar IRAS 16293–2422 as told by the cyanopolyynes

Astronomy and astrophysics (Berlin), 2017-01, Vol.597, p.A40

2017

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Dust formation around AGB and SAGB stars: a trend with metallicity?

Monthly notices of the Royal Astronomical Society, 2012-08, Vol.424 (3), p.2345-2357

2012

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Ice and Dust in the Quiescent Medium of Isolated Dense Cores

The Astrophysical journal, 2011-03, Vol.729 (2), p.92-jQuery1323910290567='48'

2011

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ab-Initio and DFT study of HCN: Role of temperature for the formation of HCN molecule in the interstellar medium

Journal of molecular structure, 2022-01, Vol.1248, p.131460, Article 131460

2022

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DISCOVERY OF ENHANCED RADIATIVE RECOMBINATION CONTINUA OF He-LIKE IRON AND CALCIUM FROM IC 443 AND ITS IMPLICATIONS

The Astrophysical journal, 2014-03, Vol.784 (1), p.1-4

2014

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Monte Carlo method for calculating oxygen abundances and their uncertainties from strong-line flux measurements

Astronomy and computing, 2016-07, Vol.16, p.54-66

2016

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Metal abundances in the MACER simulations of the hot interstellar medium

Astronomische Nachrichten, 2020-02, Vol.341 (2), p.184-190

2020

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Condensed Matter Astrophysics: A Prescription for Determining the Species-specific Composition and Quantity of Interstellar Dust Using X-rays

The Astrophysical journal, 2009-09, Vol.702 (2), p.970-979

2009

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Deriving model-based Te-consistent chemical abundances in ionized gaseous nebulae

Monthly notices of the Royal Astronomical Society, 2014-05, Vol.441 (3), p.2663-2675

Perez-Montero, E.

2014

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A Unified Representation of Gas-Phase Element Depletions in the Interstellar Medium

The Astrophysical journal, 2009-08, Vol.700 (2), p.1299-1348

Jenkins, Edward B

2009

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Early-type stars observed in the ESO UVES Paranal Observatory Project – IV. Studies of CN, CH+ and CH in the interstellar medium

Monthly notices of the Royal Astronomical Society, 2014-02, Vol.438 (2), p.1127-1136

2014

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The Te[N ii]–Te[O iii] temperature relation in H ii regions and the reliability of strong-line methods

Monthly notices of the Royal Astronomical Society, 2020-09, Vol.497 (1), p.672-686

2020

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A Three-Position Spectral Line Survey of Sagittarius B2 between 218 and 263 GHz. II. Data Analysis

The Astrophysical journal. Supplement series, 2000-05, Vol.128 (1), p.213-243

2000

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Chains of dense cores in the Taurus L1495/B213 complex

CONSTRAINING THE ABUNDANCES OF COMPLEX ORGANICS IN THE INNER REGIONS OF SOLAR-TYPE PROTOSTARS

The Case of H2C3O Isomers, Revisited: Solving the Mystery of the Missing Propadienone

Hydrodynamics with gas–grain chemistry and radiative transfer: comparing dynamical and static models

Dust Destruction in Nonradiative Shocks

Is the Gas-phase OH+H2CO Reaction a Source of HCO in Interstellar Cold Dark Clouds? A Kinetic, Dynamic, and Modeling Study

Galactic Chemical Evolution of Radioactive Isotopes

Water deuterium fractionation in the high-mass star-forming region G34.26+0.15 based on Herschel/HIFI data

Spitzer Observations of HH 54 and HH 7-11: Mapping the H2 Ortho-to-Para Ratio in Shocked Molecular Gas

Ortho-to-para ratio of NH2. Herschel-HIFI observations of ortho- and para-NH2 rotational transitions towards W31C, W49N, W51 and G34.3+0.1

Effect of the Surface Roughness of Icy Grains on Molecular Oxygen Chemistry in Molecular Clouds

History of the solar-type protostar IRAS 16293–2422 as told by the cyanopolyynes

Dust formation around AGB and SAGB stars: a trend with metallicity?

Ice and Dust in the Quiescent Medium of Isolated Dense Cores

Herschel observations of EXtra-Ordinary Sources (HEXOS): Methanol as a probe of physical conditions in Orion KL

ab-Initio and DFT study of HCN: Role of temperature for the formation of HCN molecule in the interstellar medium

DISCOVERY OF ENHANCED RADIATIVE RECOMBINATION CONTINUA OF He-LIKE IRON AND CALCIUM FROM IC 443 AND ITS IMPLICATIONS

Monte Carlo method for calculating oxygen abundances and their uncertainties from strong-line flux measurements

Metal abundances in the MACER simulations of the hot interstellar medium

Condensed Matter Astrophysics: A Prescription for Determining the Species-specific Composition and Quantity of Interstellar Dust Using X-rays

Deriving model-based Te-consistent chemical abundances in ionized gaseous nebulae

A Unified Representation of Gas-Phase Element Depletions in the Interstellar Medium

Early-type stars observed in the ESO UVES Paranal Observatory Project – IV. Studies of CN, CH+ and CH in the interstellar medium

The Te[N ii]–Te[O iii] temperature relation in H ii regions and the reliability of strong-line methods

A Three-Position Spectral Line Survey of Sagittarius B2 between 218 and 263 GHz. II. Data Analysis

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