Search for dissertations about: "interstellar-medium"

Showing result 1 - 5 of 71 swedish dissertations containing the word interstellar-medium.

  2. 1. Observations and astrophysical modelling of the interstellar medium

    Author : Achim Tappe; Chalmers tekniska högskola; []
    Keywords : NATURVETENSKAP; NATURAL SCIENCES; ISM:individual: Gum nebula ; emmission lines; quasars: individual: PKS B2145 067 ; HII regions; quasars: absorption lines; interstellar medium ISM : general; stars: individual: Zeta Puppis ;

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  4. 2. Interstellar molecules in the Magellanic clouds

    Author : Arto Heikkilä; Chalmers tekniska högskola; []
    Keywords : NATURVETENSKAP; NATURAL SCIENCES; abundances; interstellar medium: molecules; galaxies: interstellar medium; magellanic clouds; abundances;

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  5. 3. Studies of Interstellar Molecular Gas in the Magellanic Clouds

    Author : Arto Heikkilä; Chalmers tekniska högskola; []
    Keywords : NATURVETENSKAP; NATURAL SCIENCES; TEKNIK OCH TEKNOLOGIER; ENGINEERING AND TECHNOLOGY; abundances-Galaxies; evolution; molecules-Galaxies; Magellanic Clouds-Interstellar medium; molecules-Galaxies; interstellar medium-Galaxies;

    Abstract : Results of observational studies of interstellar molecular gas clouds in the Large Magellanic Cloud (LMC) and the Small Magellanic Cloud (SMC), two nearby metal-poor and dust-poor dwarf galaxies, are presented. Spectral line radiation emitted by interstellar molecules has been used to probe the physical state and the chemical composition of individual molecular clouds. READ MORE

  6. 4. Radio recombination and molecular lines in the interstellar medium

    Author : B. Torgny Cato; Chalmers tekniska högskola; []
    Keywords : NATURVETENSKAP; NATURAL SCIENCES;

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  7. 5. Ionized and atomic interstellar medium in star-forming galaxies

    Author : Thøger Emil Rivera-Thorsen; Göran Östlin; Matthew Hayes; Dawn Erb; Stockholms universitet; []
    Keywords : NATURVETENSKAP; NATURAL SCIENCES; Astronomy; astronomi;

    Abstract : Star forming galaxies in the local Universe are an important laboratory for learning about conditions in the distant, early Universe. With a high frequency of interactions and mergers, strong star formation activity, and complex kinematics and often disturbed or irregular morphology, these galaxies are believed to be the best local analogs to the galaxies at early times, and can therefore help understand the galaxies we observe at high redshifts in the early Universe. READ MORE