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Volumn 143, Issue 1-4, 2009, Pages 311-322

The origins and physical properties of the complex of local interstellar clouds

a HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS (United States)

Author keywords

Interstellar medium: Atomic processes; Interstellar medium: Physical properties; Interstellar medium: Solar neighborhood

Indexed keywords

CLOUDS; CONVOLUTION; DUST; GAS ABSORPTION; IONIZATION OF GASES; PHYSICAL PROPERTIES; SILICATES; SOLAR EQUIPMENT; STARS;

A DENSITIES; ABSORPTION LINES; AMBIENT MEDIUMS; CARBONACEOUS GRAINS; ELECTRON DENSITIES; HELIOSPHERE; IN-SITU OBSERVATIONS; INTERSTELLAR GAS; INTERSTELLAR MEDIUM: ATOMIC PROCESSES; INTERSTELLAR MEDIUM: PHYSICAL PROPERTIES; INTERSTELLAR MEDIUM: SOLAR NEIGHBORHOOD; INTERSTELLAR RADIATIONS; LINES OF SIGHTS; LOCAL INTERSTELLAR CLOUDS; LOW DENSITIES; NON EQUILIBRIUMS; THEORETICAL MODELING;

SOLAR SYSTEM;

EID: 61449149711 PISSN: 00386308 EISSN: 15729672 Source Type: Journal
DOI: 10.1007/s11214-008-9342-3 Document Type: Article

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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.