Search Results - Ibáñez-Mejía, Juan C.

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  1. 1
    Feeding versus Falling: The Growth and Collapse of Molecular Clouds in a Turbulent Interstellar Medium

    Feeding versus Falling: The Growth and Collapse of Molecular Clouds in a Turbulent Interstellar Medium by Ibáñez-Mejía, Juan C., Mac Low, Mordecai-Mark, Klessen, Ralf S., Baczynski, Christian

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  2. 2
    Effect of the Heating Rate on the Stability of the Three-phase Interstellar Medium

    Effect of the Heating Rate on the Stability of the Three-phase Interstellar Medium by Hill, Alex S., Mac Low, Mordecai-Mark, Gatto, Andrea, Ibáñez-Mejía, Juan C.

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  3. 3
    Use and abuse of detrital zircon U-Pb geochronology; a case from the Rio Orinoco Delta, eastern Venezuela

    Use and abuse of detrital zircon U-Pb geochronology; a case from the Rio Orinoco Delta, eastern Venezuela by Ibañez-Mejia, Mauricio, Pullen, Alex, Pepper, Martin, Urbani, Franco, Ghoshal, Gourab, Ibañez-Mejia, Juan C

    Published in Geology (Boulder)
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  4. 4
    GRAVITATIONAL CONTRACTION VERSUS SUPERNOVA DRIVING AND THE ORIGIN OF THE VELOCITY DISPERSION-SIZE RELATION IN MOLECULAR CLOUDS

    GRAVITATIONAL CONTRACTION VERSUS SUPERNOVA DRIVING AND THE ORIGIN OF THE VELOCITY DISPERSION-SIZE RELATION IN MOLECULAR CLOUDS by Ibáñez-Mejía, Juan C., Mac Low, Mordecai-Mark, Klessen, Ralf S., Baczynski, Christian

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  5. 5
    Gravity versus Magnetic Fields in Forming Molecular Clouds

    Gravity versus Magnetic Fields in Forming Molecular Clouds by Ibáñez-Mejía, Juan C., Mac Low, Mordecai-Mark, Klessen, Ralf S.

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  6. 6
    What happens when n= 1000? Creating large-n geochronological datasets with LA-ICP-MS for geologic investigationsElectronic supplementary information (ESI) available. See DOI: 10.1039/c4ja00024b

    What happens when n= 1000? Creating large-n geochronological datasets with LA-ICP-MS for geologic investigationsElectronic supplementary information (ESI) available. See DOI: 10.10... by Pullen, Alex, Ibáñez-Mejía, Mauricio, Gehrels, George E, Ibáñez-Mejía, Juan C, Pecha, Mark

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  7. 7
    Fast Molecular Cloud Destruction Requires Fast Cloud Formation

    Fast Molecular Cloud Destruction Requires Fast Cloud Formation by Mac Low, Mordecai-Mark, Burkert, Andreas, Ibáñez-Mejía, Juan C.

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  8. 8
    What happens when n= 1000? Creating large-n geochronological datasets with LA-ICP-MS for geologic investigations

    What happens when n= 1000? Creating large-n geochronological datasets with LA-ICP-MS for geologic investigations by Pullen, Alex, Ibáñez-Mejía, Mauricio, Gehrels, George E., Ibáñez-Mejía, Juan C., Pecha, Mark

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  9. 9
    Dust charge distribution in the interstellar medium

    Dust charge distribution in the interstellar medium by Ibáñez-Mejía, Juan C, Walch, Stefanie, Ivlev, Alexei V, Clarke, Seamus, Caselli, Paola, Joshi, Prabesh R

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  10. 10
    GRAVITATIONAL CONTRACTION VERSUS SUPERNOVA DRIVING AND THE ORIGIN OF THE VELOCITY DISPERSION–SIZE RELATION IN MOLECULAR CLOUDS

    GRAVITATIONAL CONTRACTION VERSUS SUPERNOVA DRIVING AND THE ORIGIN OF THE VELOCITY DISPERSION–SIZE RELATION IN MOLECULAR CLOUDS by Ibáñez-Mejía, Juan C., Mac Low, Mordecai-Mark, Klessen, Ralf S., Baczynski, Christian

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  11. 11
    Gravity Versus Magnetic Fields in Forming Molecular Clouds

    Gravity Versus Magnetic Fields in Forming Molecular Clouds by Ibáñez-Mejía, Juan C, Mordecai-Mark Mac Low, Klessen, Ralf S

    Published in arXiv.org
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  12. 12
    Dust charge distribution in the interstellar medium

    Dust charge distribution in the interstellar medium by Ibáñez-Mejía, Juan C, Walch, Stefanie, Ivlev, Alexei V, Clarke, Seamus, Caselli, Paola, Joshi, Prabesh R

    Published in arXiv.org
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  13. 13
    Feeding vs. Falling: The growth and collapse of molecular clouds in a turbulent interstellar medium

    Feeding vs. Falling: The growth and collapse of molecular clouds in a turbulent interstellar medium by Ibáñez-Mejía, Juan C, Mordecai-Mark Mac Low, Klessen, Ralf S, Baczynski, Christian

    Published in arXiv.org
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  14. 14
    Fast Molecular Cloud Destruction Requires Fast Cloud Formation

    Fast Molecular Cloud Destruction Requires Fast Cloud Formation by Mordecai-Mark Mac Low, Burkert, Andreas, Ibáñez-Mejía, Juan C

    Published in arXiv.org
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  15. 15
    Effect of the heating rate on the stability of the three-phase interstellar medium

    Effect of the heating rate on the stability of the three-phase interstellar medium by Hill, Alex S, Mordecai-Mark Mac Low, Gatto, Andrea, Ibáñez-Mejía, Juan C

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  16. 16
    What happens when n= 1000? Creating large-ngeochronological datasets with LA-ICP-MS for geologic investigations

    What happens when n= 1000? Creating large-ngeochronological datasets with LA-ICP-MS for geologic investigations by Pullen, Alex, Ibanez-Mejia, Mauricio, Gehrels, George E, Ibanez-Mejia, Juan C, Pecha, Mark

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  17. 17
    Gravitational contraction versus Supernova driving and the origin of the velocity dispersion-size relation in molecular clouds

    Gravitational contraction versus Supernova driving and the origin of the velocity dispersion-size relation in molecular clouds by Ibáñez-Mejía, Juan C, Mordecai-Mark Mac Low, Klessen, Ralf S, Baczynski, Christian

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  18. 18
    Stability of toroidal magnetic fields in stellar interiors

    Stability of toroidal magnetic fields in stellar interiors by Ibañez-Mejia, Juan C, Braithwaite, Jonathan

    Published in arXiv.org
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