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Gamma-Ray Astronomy
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Gamma-Ray Astronomy - pocketboek

1976, ISBN: 9789027706966

Observation of discrete energy electromagnetic emissions from celestial objects in the radio, IR, optical, lN, and X-ray spectral regions has dramatically advanced our know ledge in the … Meer...

Nr. 4683047. Verzendingskosten:, Lieferbar in 2 - 3 Tage, DE. (EUR 0.00)

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E. L. Chupp,:

Gamma-Ray Astronomy. E. L. Chupp, - Buch - nieuw boek

ISBN: 9789027706966

Gamma-Ray Astronomy. Observation of discrete energy electromagnetic emissions from celestial objects in the radio, IR, optical, lN, and X-ray spectral regions has dramatically advanced ou… Meer...

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Chupp, E. L.:
Gamma-Ray Astronomy - pocketboek

ISBN: 9789027706966

Erscheinungsdatum: 31.12.1976, Medium: Taschenbuch, Einband: Kartoniert / Broschiert, Titel: Gamma-Ray Astronomy, Titelzusatz: Nuclear Transition Region, Auflage: Softcover reprint of the… Meer...

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E.L. Chupp:
Gamma-Ray Astronomy - nieuw boek

ISBN: 9789027706966

Physics; Astronomy, Observations and Techniques Supernova, astronomy, astrophysics, black hole, black holes, cosmic ray, instruments, neutron star, telescope, universe Books, Springer Shop

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E. L. Chupp:
Gamma-Ray Astronomy - pocketboek

1976, ISBN: 9789027706966

Nuclear Transition Region, Softcover reprint of the original 1st ed. 1976, Softcover, Buch, [PU: Kluwer Academic Publishers]

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Bijzonderheden over het boek
Gamma Ray Astronomy

Observation of discrete energy electromagnetic emissions from celestial objects in the radio, IR, optical, lN, and X-ray spectral regions has dramatically advanced our know­ ledge in the field of astrophysics. It is expected that identification of nuclear 'Y-ray line emissions from any cosmic source would also prove to be a powerful new tool for probing the Universe. Since the publication of Morrison's work in 1958, many experiments were carried out searching for evidence of 'Y-ray lines from cosmic sources, however with little success. Only a few positive experimental results have been reported, in spite of an expenditure of considerable effort by many people: in particular, the possible Galactic Center emission line (473 to 530keV) and 'Y-ray lines at several energies (e. g. , 0. 5 MeV and 2. 2 MeV) associated with large solar flares. Both of these observations are unconfirmed by indepen­ dent observations (ca. 1975). The high energy 'Y-rays (>30MeV) from the Galactic Center are at least partly due to the decay of 1[0 mesons, which are of unique energy (67. 5 MeV) in the 1[0 rest frame only. The reasons for the limited amount of data avail­ able in this field, even though early theoretical predictions were very optimistic regarding fluxes of nuclear lines, are that experimental efforts are plagued with high backgrounds and low fluxes, and that development of instruments with telescopic properties in the energy range of interest is difficult.

Gedetalleerde informatie over het boek. - Gamma Ray Astronomy


EAN (ISBN-13): 9789027706966
ISBN (ISBN-10): 9027706964
Gebonden uitgave
pocket book
Verschijningsjaar: 1976
Uitgever: Springer-Verlag GmbH
336 Bladzijden
Gewicht: 0,504 kg
Taal: eng/Englisch

Boek bevindt zich in het datenbestand sinds 2007-07-20T23:50:01+02:00 (Amsterdam)
Detailpagina laatst gewijzigd op 2020-08-24T11:23:35+02:00 (Amsterdam)
ISBN/EAN: 9027706964

ISBN - alternatieve schrijfwijzen:
90-277-0696-4, 978-90-277-0696-6


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