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What makes a planet habitable?

The Astronomy and astrophysics review, 2009-06, Vol.17 (2), p.181-249

2009

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In-situ chemical investigation of a comet nucleus by gas chromatography : Porous layer open tubular columns for the separation of light, volatile compounds

Chromatographia, 2001-09, Vol.54 (5-6), p.369-376

2001

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Atmospheric nitrogen fixation rate by lightning and coronae discharges over the earth's geologic history

Origins of life and evolution of biospheres, 2002-12, Vol.32 (5-6), p.408-408

2002

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Nitrogen fixation by corona discharge on the early precambrian Earth

Origins of life and evolution of biospheres, 2005-10, Vol.35 (5), p.401-409

2005

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Identification of amino acids by capillary gas chromatography. Application to martian samples

Chromatographia, 2001, Vol.53 (S1), p.S332-S339

2001

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Temperature dependence of HC3N, C6H2, and C4N2 mid-UV absorption coefficients. Application to the interpretation of Titan's atmospheric spectra

Astrophysics and space science, 1996, Vol.236 (1), p.85-95

1996

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Sensitivity effects of chemical kinetic uncertainties on photochemical modeling results : Application to Titan's atmosphere

Origins of life and evolution of biospheres, 2006-06, Vol.36 (3), p.332-333

2006

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Review and latest results of laboratory investigations of Titan's aerosols

Origins of life and evolution of biospheres, 1998-04, Vol.28 (2), p.195-213

1998

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The role of sulphur in chemical evolution

Journal of molecular evolution, 1977-12, Vol.9 (4), p.329-338

1977

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Effect of H2S on the formation of organic compounds from C, N,H, S model atmospheres submitted to a glow discharge

Origins of Life, 1975-10, Vol.6 (4), p.507-512

1975

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Formation of prebiochemical compounds in models of the primitive earth's atmosphere. II: CH4 - H2S atmospheres

Origins of life, 1975-01, Vol.6 (1-2), p.91

1975

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Far UV irradiation of model prebiotic atmospheres

Origins of Life, 1977-10, Vol.8 (3), p.259-266

1977

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Exobiology and the solar system: the Cassini mission to Titan

Origins of Life, 1984-01, Vol.14 (1-4), p.817-824

1984

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From Panspermia to Bioastronomy, the evolution of the hypothesis of universal life

Origins of life and evolution of biospheres, 1998-10, Vol.28 (4-6), p.597-612

1998

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Formation of prebiochemical compounds in models of the primitive earth's atmosphere. I: CH4 NH3 and CH4 N2 atmospheres

Origins of Life, 1975-01, Vol.6 (1-2), p.83-90

1975

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Exobiology on Titan: A reference laboratory for studying prebiotic chemistry on a planetary scale

Journal of biological physics, 1995-03, Vol.20 (1-4), p.39-53

1995

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Temperature dependence of HC sub(3) N, C sub(6) H sub(2) , and C sub(4) N sub(2) mid-UV absorption coefficients. Application to the interpretation of Titan's atmospheric spectra

Astrophysics and space science, 1996-01, Vol.236 (1), p.85-95

1996

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Investigation on Planetary Atmospheres Using Laboratory Simulation Experiments The Example of Saturn's Moon (Titan)

Earth, moon, and planets, 1998-12, Vol.80 (1-3), p.113-133

1998

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The application of electrochemical methods to the study of the electroless nickel deposition from hypophosphite solutions

Journal of applied electrochemistry, 1971-08, Vol.1 (3), p.167-177

1971

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Life in the Universe Paris, November 19?21, 1979

Origins of Life, 1980-12, Vol.10 (4), p.371-377

Raulin, Francois

1980

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Application of Electrochemical Methods to the Study of the Electroless Ni Deposition From Hypophosphite Solutions

Journal of applied electrochemistry, 1971-08, Vol.1 (3), p.167-177

1971

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Formation of prebiochemical compounds in models of the primitive Earth's atmosphere: II: CH4?H2SAtmospheres

Origins of Life, 1975-01, Vol.6 (1-2), p.91-97

1975

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Titan's ocean

Origins of life and evolution of biospheres, 1989-05, Vol.19 (3-5), p.471-472

1989

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Infrared spectra of gas phase organics : New data and implication for Titan's atmosphere

Origins of life and evolution of biospheres, 1989-05, Vol.19 (3-5), p.499-500

1989

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Organic synthesis from reducing models of the atmosphere of the primitive earth with UV light and electric discharges

Journal of molecular evolution, 1982-01, Vol.18 (3), p.173-178

1982

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What makes a planet habitable?

In-situ chemical investigation of a comet nucleus by gas chromatography : Porous layer open tubular columns for the separation of light, volatile compounds

Atmospheric nitrogen fixation rate by lightning and coronae discharges over the earth's geologic history

Nitrogen fixation by corona discharge on the early precambrian Earth

Identification of amino acids by capillary gas chromatography. Application to martian samples

Temperature dependence of HC3N, C6H2, and C4N2 mid-UV absorption coefficients. Application to the interpretation of Titan's atmospheric spectra

Sensitivity effects of chemical kinetic uncertainties on photochemical modeling results : Application to Titan's atmosphere

Review and latest results of laboratory investigations of Titan's aerosols

The role of sulphur in chemical evolution

Effect of H2S on the formation of organic compounds from C, N,H, S model atmospheres submitted to a glow discharge

Formation of prebiochemical compounds in models of the primitive earth's atmosphere. II: CH4 - H2S atmospheres

Far UV irradiation of model prebiotic atmospheres

Exobiology and the solar system: the Cassini mission to Titan

From Panspermia to Bioastronomy, the evolution of the hypothesis of universal life

Formation of prebiochemical compounds in models of the primitive earth's atmosphere. I: CH4 NH3 and CH4 N2 atmospheres

Exobiology on Titan: A reference laboratory for studying prebiotic chemistry on a planetary scale

Temperature dependence of HC sub(3) N, C sub(6) H sub(2) , and C sub(4) N sub(2) mid-UV absorption coefficients. Application to the interpretation of Titan's atmospheric spectra

Investigation on Planetary Atmospheres Using Laboratory Simulation Experiments The Example of Saturn's Moon (Titan)

The application of electrochemical methods to the study of the electroless nickel deposition from hypophosphite solutions

Life in the Universe Paris, November 19?21, 1979

Application of Electrochemical Methods to the Study of the Electroless Ni Deposition From Hypophosphite Solutions

Formation of prebiochemical compounds in models of the primitive Earth's atmosphere: II: CH4?H2SAtmospheres

Titan's ocean

Infrared spectra of gas phase organics : New data and implication for Titan's atmosphere

Organic synthesis from reducing models of the atmosphere of the primitive earth with UV light and electric discharges

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