Author: L. Pocs
Publisher:
ISBN:
Category : Controlled fusion
Languages : en
Pages : 772
Book Description
12th European Conference on Controlled Fusion and Plasma Physics, Budapest, 2-6 September 1985
Author: L. Pocs
Publisher:
ISBN:
Category : Controlled fusion
Languages : en
Pages : 772
Book Description
Publisher:
ISBN:
Category : Controlled fusion
Languages : en
Pages : 772
Book Description
Energy Research Abstracts
Author:
Publisher:
ISBN:
Category : Power resources
Languages : en
Pages : 1076
Book Description
Publisher:
ISBN:
Category : Power resources
Languages : en
Pages : 1076
Book Description
Physics Briefs
Author:
Publisher:
ISBN:
Category : Physics
Languages : en
Pages : 862
Book Description
Publisher:
ISBN:
Category : Physics
Languages : en
Pages : 862
Book Description
13th European Conference on Controlled Fusion and Plasma Heating, Schliersee, 14-18 April 1986
Author:
Publisher:
ISBN:
Category : Controlled fusion
Languages : en
Pages : 460
Book Description
Publisher:
ISBN:
Category : Controlled fusion
Languages : en
Pages : 460
Book Description
Fusion Energy Update
Author:
Publisher:
ISBN:
Category : Controlled fusion
Languages : en
Pages : 100
Book Description
Publisher:
ISBN:
Category : Controlled fusion
Languages : en
Pages : 100
Book Description
Scientific and Technical Aerospace Reports
Author:
Publisher:
ISBN:
Category : Aeronautics
Languages : en
Pages : 1162
Book Description
Publisher:
ISBN:
Category : Aeronautics
Languages : en
Pages : 1162
Book Description
Polycyclic Aromatic Hydrocarbons and Astrophysics
Author: A. Léger
Publisher: Springer Science & Business Media
ISBN: 9400947763
Category : Science
Languages : en
Pages : 405
Book Description
The near Infra-Red emission of the Interstellar Medium is a very puzzling subject. In the brightest regions, where spectroscopic observa tions are possible from the ground, several bands (3.3 - 3.4 - 6.2 - 7.7 - 8.6 - 11.3 ~m) have been observed since 1973. The absence of satisfying explanation was so obvious that they were called "Unidenti fied IR Emission Bands". The puzzle still increased when were known the first results of the general IR sky survey made by the satellite IRAS. On a large scale, the near IR emission of the Interstellar medium was expected to be very small but it was observed to be about one third of the total IR emission for our own galaxy ..• The situation has moved in 1984 when it was suggested that a class of stable organic molecules, the Polycyclic Aromatic Hydrocarbons (PAH's) could be at the origin of this near IR emission. Initially based on the required refractory character of particules that should be heated to high temperature without subliming, this hypothesis leads to a sugges tive spectroscopic similarity with the observed astronomical bands. This hypothesis is attractive and it has many implications, for ins tance, the PAHs would be the most abundant organic molecules in the universe. However, many points have to be clarified and the different consequences of this suggestion should be explored.
Publisher: Springer Science & Business Media
ISBN: 9400947763
Category : Science
Languages : en
Pages : 405
Book Description
The near Infra-Red emission of the Interstellar Medium is a very puzzling subject. In the brightest regions, where spectroscopic observa tions are possible from the ground, several bands (3.3 - 3.4 - 6.2 - 7.7 - 8.6 - 11.3 ~m) have been observed since 1973. The absence of satisfying explanation was so obvious that they were called "Unidenti fied IR Emission Bands". The puzzle still increased when were known the first results of the general IR sky survey made by the satellite IRAS. On a large scale, the near IR emission of the Interstellar medium was expected to be very small but it was observed to be about one third of the total IR emission for our own galaxy ..• The situation has moved in 1984 when it was suggested that a class of stable organic molecules, the Polycyclic Aromatic Hydrocarbons (PAH's) could be at the origin of this near IR emission. Initially based on the required refractory character of particules that should be heated to high temperature without subliming, this hypothesis leads to a sugges tive spectroscopic similarity with the observed astronomical bands. This hypothesis is attractive and it has many implications, for ins tance, the PAHs would be the most abundant organic molecules in the universe. However, many points have to be clarified and the different consequences of this suggestion should be explored.
Host Bibliographic Record for Boundwith Item Barcode 30112033097202 and Others
Author:
Publisher:
ISBN:
Category :
Languages : en
Pages : 526
Book Description
Publisher:
ISBN:
Category :
Languages : en
Pages : 526
Book Description
Physics of Mirrors, Reversed Field Pinches, and Compact Tori
Author: S. Ortolani
Publisher:
ISBN:
Category : Magnetic fields
Languages : en
Pages : 288
Book Description
Publisher:
ISBN:
Category : Magnetic fields
Languages : en
Pages : 288
Book Description
British Reports, Translations and Theses Received by the British Library Lending Division (including Material from the Republic of Ireland).
Author: British Library. Document Supply Centre
Publisher:
ISBN:
Category : Conference proceedings
Languages : en
Pages : 524
Book Description
Issue for Mar. 1981 contains index for Jan.-Mar. 1981 in microfiche form.
Publisher:
ISBN:
Category : Conference proceedings
Languages : en
Pages : 524
Book Description
Issue for Mar. 1981 contains index for Jan.-Mar. 1981 in microfiche form.