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OverviewThe 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. Full Product DetailsAuthor: Brian M Cancellieri , Vladimir G MamedovPublisher: Nova Science Publishers Inc Imprint: Nova Science Publishers Inc Dimensions: Width: 23.00cm , Height: 1.80cm , Length: 15.50cm Weight: 0.333kg ISBN: 9781614708070ISBN 10: 161470807 Pages: 202 Publication Date: 01 October 2011 Audience: College/higher education , Postgraduate, Research & Scholarly Format: Hardback Publisher's Status: Active Availability: Awaiting stock ![]() The supplier is currently out of stock of this item. It will be ordered for you and placed on backorder. Once it does come back in stock, we will ship it out for you. Table of ContentsPreface; Explosive Processes in the Interstellar Medium as Sources of Ultrahigh-Energy Cosmic Rays; Heteronuclear Diatomics in Diffuse & Translucent Clouds; Space Wing Electro AB-Ship; FUV Characteristics of the Interstellar Medium of the Large Magellanic Cloud; MHD Simulations of Parker Instability Undergoing Cosmic-Ray Diffusion; Interaction of Planetary Nebulae, Eta-Carinae & Supernova Remnants with the Interstellar Medium; Deuterium in the Interstellar Medium; Interstellar Medium; Index.ReviewsAuthor InformationTab Content 6Author Website:Countries AvailableAll regions |