Interstellar Medium: New Research

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Title: Interstellar Medium: New Research
Description: The interstellar medium (or ISM) is the matter that exists in the space between the star systems in a galaxy. This matter includes gas in ionic, atomic, and molecular form, dust, and cosmic rays. It fills interstellar space and blends smoothly into the surrounding intergalactic space. This book presents topical research in the study of interstellar medium, including explosive processes in the interstellar medium as sources of ultrahigh-energy cosmic rays; heteronuclear diatomics in diffuse and translucent clouds; far ultraviolet observations of the Large Magellanic Cloud; MDH simulations of Parker instability undergoing cosmic-ray diffusion; deuterium in the interstellar medium and interaction of planetary nebulae, Eta-Carinae and supernova remnants with the interstellar medium.
Authors: Mamedov, Vladimir G., Cancellieri, Brian M.
Resource Type: eBook.
Subjects: Interstellar matter
Categories: SCIENCE / Space Science / Astronomy
Database: eBook Collection (EBSCOhost)
FullText Links:
  – Type: ebook-pdf
Text:
  Availability: 0
Header DbId: nlebk
DbLabel: eBook Collection (EBSCOhost)
An: 666149
RelevancyScore: 1044
AccessLevel: 6
PubType: eBook
PubTypeId: ebook
PreciseRelevancyScore: 1044.26904296875
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Items – Name: Title
  Label: Title
  Group: Ti
  Data: Interstellar Medium: New Research
– Name: Abstract
  Label: Description
  Group: Ab
  Data: The interstellar medium (or ISM) is the matter that exists in the space between the star systems in a galaxy. This matter includes gas in ionic, atomic, and molecular form, dust, and cosmic rays. It fills interstellar space and blends smoothly into the surrounding intergalactic space. This book presents topical research in the study of interstellar medium, including explosive processes in the interstellar medium as sources of ultrahigh-energy cosmic rays; heteronuclear diatomics in diffuse and translucent clouds; far ultraviolet observations of the Large Magellanic Cloud; MDH simulations of Parker instability undergoing cosmic-ray diffusion; deuterium in the interstellar medium and interaction of planetary nebulae, Eta-Carinae and supernova remnants with the interstellar medium.
– Name: Author
  Label: Authors
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  Data: <searchLink fieldCode="AR" term="%22Mamedov%2C+Vladimir+G%2E%22">Mamedov, Vladimir G.</searchLink><br /><searchLink fieldCode="AR" term="%22Cancellieri%2C+Brian+M%2E%22">Cancellieri, Brian M.</searchLink>
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  Data: eBook.
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  Data: <searchLink fieldCode="DE" term="%22Interstellar+matter%22">Interstellar matter</searchLink>
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  Data: <searchLink fieldCode="ZK" term="%22SCIENCE+%2F+Space+Science+%2F+Astronomy%22">SCIENCE / Space Science / Astronomy</searchLink>
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RecordInfo BibRecord:
  BibEntity:
    Classifications:
      – Code: 523.1135
        Scheme: ddc
        Type: prePub
    Languages:
      – Code: eng
        Text: English
    Subjects:
      – SubjectFull: Interstellar matter
        Type: general
    Titles:
      – TitleFull: Interstellar Medium: New Research
        Type: main
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      – PersonEntity:
          Name:
            NameFull: Mamedov, Vladimir G.
      – PersonEntity:
          Name:
            NameFull: Cancellieri, Brian M.
      – PersonEntity:
          Name:
            NameFull: Mamedov, Vladimir G.
      – PersonEntity:
          Name:
            NameFull: Cancellieri, Brian M.
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          Dates:
            – D: 01
              M: 01
              Type: published
              Y: 2012
            – D: 04
              M: 02
              Type: profile
              Y: 2014
          Identifiers:
            – Type: isbn-print
              Value: 9781614708070
            – Type: isbn-electronic
              Value: 9781614708599
          Titles:
            – TitleFull: Interstellar Medium: New Research
              Type: main
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