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         Interstellar Medium:     more books (100)
  1. The Interstellar Medium in Galaxies (Astrophysics and Space Science Library)
  2. Triggered Star Formation in a Turbulent Interstellar Medium (IAU S237) (Proceedings of the International Astronomical Union Symposia and Colloquia)
  3. Star Formation, Galaxies and the Interstellar Medium
  4. Supernovae and Stellar Wind in the Interstellar Medium (Translation Series) by Tatjana A. Lozinskaya, 1991-11-01
  5. Interstellar Turbulence
  6. Evolution of Interstellar Matter and Dynamics of Galaxies (Center for Theoretic)
  7. Astrochemistry: Carl Sagan, Timeline of Knowledge About the Interstellar and Intergalactic Medium, Interstellar Medium
  8. Astronomical Objects: Constellation, Interstellar Medium, Outer Space, Cosmic Dust, Asterism, Stellar Magnetic Field, Astronomical Symbols
  9. Cosmic Dust: Dust, Molecule, Outer space, Interstellar medium, Nebula, Circumstellar disk, Planetary ring, Zodiacal light, Comet dust, Asteroid belt, Kuiper ... nucleosynthesis, Interplanetary dust cloud
  10. High Energy Astrophysics Stars the Galaxy and Interstellar Medium - 2nd Edition by MSLongair, 1994
  11. The final chemistry frontier: molecules of the interstellar medium must break the rules to make the stuff of space.: An article from: Science News by Rachel Ehrenberg, 2010-01-30
  12. Tetons 4; Galactic Structure, Stars, and the Interstellar Medium; Proceedings. by Charles E. Woodward Et Al, 1980
  13. Stars, Nebulae and the Interstellar Medium: Observational Physics and Astrophysics by C. R. Kitchin, 1987
  14. LOCAL INTERSTELLAR MEDIUM, Proceedings of the International Astronomical Union's Colloquium Number 81, 4-6 June 1984, Madison, Wisconsin, NASA CP-2345 by Y.; Bruhweiler, F. C.; Savage, B. D. (Eds) Kondo, 1984

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    47. Interstellar Medium / Research @ CITA / CITA
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    Interstellar Medium Related CITA preprints Stars and the interstellar medium are the two components of the Galaxy, and they have a close and intricate relationship. Stars form out of clouds of gas and dust. Stellar radiation and winds, as well as supernova explosions, play crucial roles in sculpting the ISM. The Canadian Galactic Plane Survey, for which Martin serves as a scientific director, is conducting an HI and continuum radio survey at 1 arc minute resolution. Combined with other data sets with similar resolution, this provides an excellent resource for studying the interplay between stars and the ISM. Much of the ISM-related research at CITA focusses on the process of star formation. We know that stars form when dense "cores" within molecular clouds collapse under their own self-gravity, but the details of the collapse have not yet been elucidated. Magnetic fields appear to play an important role. Recent Related Preprints
    Molecular Cloud Evolution. II. From Cloud Formation to the Early Stages of Star Formation in Decaying Conditions

    48. Interstellar Medium
    The interstellar medium (or ISM) is the name astronomers give to the tenuous gas and dust that pervade interstellar space. Whilst the ISM refers to the
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    Interstellar medium
    The interstellar medium (or ISM) is the name astronomers give to the tenuous gas and dust that pervade interstellar space. See also: Whilst the ISM refers to the matter (interstellar matter, also abbreviated by ISM) that exists between the stars within a galaxy, the energy, in the form of electromagnetic radiation, that occupies the same volume is called the interstellar radiation field (or ISRF). The ISM consists of an extremely dilute (by terrestrial standards) plasma, gas and dust, consisting of a mixture of ions, atoms, molecules, larger dust grains, electromagnetic radiation, cosmic rays, and magnetic fields. The matter consists of about 99% gas and 1% dust by mass. It fills interstellar space. This mixture is usually extremely tenuous, with typical gas densities ranging from a few hundred to a few hundred million particles per cubic meter. As a result of primordial nucleosynthesis, the gas is roughly 90% hydrogen and 10% helium by number, with additional elements ("metals" in astronomical parlance) present in trace amounts. The ISM plays a crucial role in astrophysics precisely because of its intermediate role between stellar and galactic scales. Stars form within the densest regions of the ISM, molecular clouds, and replenish the ISM with matter and energy through planetary nebulae, stellar winds, and supernovae.

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    This article is about interstellar medium. For Steven Spielberg's upcoming sci-fi film, see Interstellar (film)
    The distribution of ionized hydrogen (known by astronomers as H II (aitch two) from old spectroscopic terminology) in the parts of the Galactic interstellar medium visible from the Earth's northern hemisphere (from the Wisconsin H-Alpha Mapper Survey) In astronomy , the interstellar medium (or ISM ) is the matter interstellar matter , also abbreviated by ISM ) and energy interstellar radiation field ISRF ) content that exists between the stars within a galaxy . The ISM plays a crucial role in astrophysics precisely because of its intermediate role between stellar and galactic scales. Stars form within the densest regions of the ISM, molecular clouds, and replenish the ISM with matter and energy through planetary nebulae stellar winds , and supernovae . In turn, this interplay between stars and the ISM helps determine the rate at which a galaxy depletes its gaseous content, and therefore its lifespan of active star formation. The ISM consists of an extremely dilute (by terrestrial standards) plasma gas and dust , consisting of a mixture of ions atoms molecules , larger dust grains electromagnetic radiation cosmic rays , and magnetic fields . The matter consists of about 99% gas and 1% dust by mass. It fills interstellar space. This mixture is usually extremely tenuous, with typical gas densities ranging from a few hundred to a few hundred million particles per cubic meter. As a result of

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    Image:Ionized-hydrogen.jpg In astronomy , the interstellar medium (or ISM ) is the matter and energy content that exists between the stars (or their immediate circumstellar environment) within a galaxy . The ISM plays a crucial role in astrophysics precisely because of its intermediate role between stellar and galactic scales. Stars themselves form within cold regions of the ISM, and replenish the ISM with matter and energy through stellar winds and supernovae . In turn, this interplay between stars and the ISM sets the rate at which a galaxy depletes its gaseous content and therefore determines its lifespan of active star formation. The ISM consists of an extremely dilute (by terrestrial standards) plasma , consisting of a mixture of atoms molecules dust electromagnetic radiation ... cosmic rays , and the magnetic field . The matter normally consists of about 99% gas particles and usually 1% dust. It fills interstellar space. This mixture is usually extremely tenuous, with typical gas densities ranging from a few single to a few hundred particles per cubic centimeter. As a result of primordial nucleosynthesis , the gas is roughly 90% hydrogen and 10% helium , with additional elements (" metals " in astronomical parlance) present in trace amounts.

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    57. Interstellar Medium - TheBestLinks.com - Galaxy, Interstellar Cloud, Kelvin, Mol
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    The interstellar medium (or ISM ) is a term used in astronomy to describe the rarefied gas and dust that exists between the stars (or their immediate "circumstellar" environment) within a galaxy . The matter normally consists of about 99% gas particles and usually 1% of dust. This compound is usually extremely tenuous, with typical densities ranging from a few single to a few hundreds of a particles per cubic centimeter. Generally the gas is roughly 90% hydrogen and 10% helium, with additional elements (" metals " in astronomical parlance) present in trace amounts. The medium is also responsible for cosmic extinction , namely the decreasing light intensity of a star as the light travels through the medium. This extinction is caused by refraction and absorption of photons in certain wavelengths. For example, the typical absorption wavelength of

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    Jump to: navigation search Image:Ionized-hydrogen.jpg The distinctive red colour emitted by warm hydrogen plasma , known as H-II (aitch two) regions, in the interplanetary medium In astronomy , the interstellar medium (or ISM ) is the matter and energy content that exists between the stars (or their immediate circumstellar environment) within a galaxy . The ISM plays a crucial role in astrophysics precisely because of its intermediate role between stellar and galactic scales. Stars themselves form within cold regions of the ISM, and replenish the ISM with matter and energy through stellar winds and supernovae . In turn, this interplay between stars and the ISM sets the rate at which a galaxy depletes its gaseous content and therefore determines its lifespan of active star formation. The ISM consists of an extremely dilute (by terrestrial standards) plasma , consisting of a mixture of atoms molecules dust electromagnetic radiation ... cosmic rays , and the magnetic field . The matter normally consists of about 99% gas particles and usually 1% dust. It fills interstellar space. This mixture is usually extremely tenuous, with typical gas densities ranging from a few single to a few hundred particles per cubic centimeter. As a result of primordial nucleosynthesis , the gas is roughly 90% hydrogen and 10% helium , with additional elements (" metals " in astronomical parlance) present in trace amounts.

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