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 Date: 2006-03-18 10:47:16Chemistry Matter Physics Chemical elements Physical cosmology Noble gases Astrochemistry Interstellar medium Hydrogen Damped Lyman-alpha system Recombination Phase transition |
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Astronomy & Astrophysics A&A 389, 393–DOI: : | Space Sci Rev: 323–331 DOIs11214Physical Properties of the Local Interstellar Medium Seth RedfieldDocID: 1uuWp - View Document |
| The Astrophysical Journal, 602:776–802, 2004 February 20 # 2004. The American Astronomical Society. All rights reserved. Printed in U.S.A. THE STRUCTURE OF THE LOCAL INTERSTELLAR MEDIUM. II. OBSERVATIONS OF D i, C ii,DocID: 1tQo8 - View Document |
| Proposal to establish a DFG priority program Physics of the Interstellar Medium Figure 1: This figure shows the star forming region NGC 602 in the Large Magellanic Cloud. Potsdam University leads a large observational pDocID: 1tQdG - View Document |
| Mon. Not. R. Astron. Soc. 000, 000–Printed 7 MarchMN LATEX style file v2.2)DocID: 1rnUh - View Document |
| CrossMark_Color_flat+clickDocID: 1rjpM - View Document |