Detection of the Water Reservoir in a Forming Planetary System-Reference-Cited by-同舟云学术

Detection of the Water Reservoir in a Forming Planetary System

Published:2011-10-21 Issue:6054 Volume:334 Page:338-340
ISSN:0036-8075
Container-title:Science
language:en
Short-container-title:Science

Author:

Hogerheijde Michiel R.¹,Bergin Edwin A.²,Brinch Christian¹,Cleeves L. Ilsedore²,Fogel Jeffrey K. J.²,Blake Geoffrey A.³,Dominik Carsten⁴,Lis Dariusz C.⁵,Melnick Gary⁶,Neufeld David⁷,Panić Olja⁸,Pearson John C.⁹,Kristensen Lars¹,Yıldız Umut A.¹,van Dishoeck Ewine F.¹¹⁰

Affiliation:

1. Leiden Observatory, Leiden University, Post Office Box 9513, 2300 RA Leiden, Netherlands.

2. Department of Astronomy, University of Michigan, Ann Arbor, MI 48109, USA.

3. Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA.

4. Astronomical Institute Anton Pannekoek, University of Amsterdam, 1098 XH Amsterdam, Netherlands.

5. Division of Physics, Mathematics, and Astronomy, California Institute of Technology, Pasadena, CA 91125, USA.

6. Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA.

7. Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD 21218, USA.

8. European Southern Observatory, 85748 Garching, Germany.

9. Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.

10. Max-Planck-Institut für Extraterrestrische Physik, 85748 Garching, Germany.

Abstract

The detection of cold water vapor in a nearby planet-forming disk suggests that water ice exists in its outer regions.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference36 articles.

1. Structure of the Solar Nebula, Growth and Decay of Magnetic Fields and Effects of Magnetic and Turbulent Viscosities on the Nebula

2. Impact-induced atmospheres and oceans on Earth and Venus

3. SPECTRALLY RESOLVED PURE ROTATIONAL LINES OF WATER IN PROTOPLANETARY DISKS

4. ORGANIC MOLECULES AND WATER IN THE INNER DISKS OF T TAURI STARS

5. Detection of Water Ice in Edge‐on Protoplanetary Disks: HK Tauri B and HV Tauri C

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