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Titlebook: Gamma-Ray Astronomy; Nuclear Transition R E. L. Chupp Book 1976 D. Reidel Publishing Company, Dordrecht, Holland 1976 Supernova.astronomy.a

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發(fā)表于 2025-3-21 17:23:08 | 只看該作者 |倒序瀏覽 |閱讀模式
書目名稱Gamma-Ray Astronomy
副標題Nuclear Transition R
編輯E. L. Chupp
視頻videohttp://file.papertrans.cn/381/380609/380609.mp4
叢書名稱Geophysics and Astrophysics Monographs
圖書封面Titlebook: Gamma-Ray Astronomy; Nuclear Transition R E. L. Chupp Book 1976 D. Reidel Publishing Company, Dordrecht, Holland 1976 Supernova.astronomy.a
描述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 t
出版日期Book 1976
關鍵詞Supernova; astronomy; astrophysics; black hole; black holes; cosmic ray; instruments; neutron star; telescop
版次1
doihttps://doi.org/10.1007/978-94-010-1496-0
isbn_softcover978-90-277-0696-6
isbn_ebook978-94-010-1496-0
copyrightD. Reidel Publishing Company, Dordrecht, Holland 1976
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Angewandte Literaturwissenschaftrence (Stecker and Trombka, 1973). Stecker (1975) has reviewed the theoretical and experimental work concerned with energetic γ-rays (> 30 MeV). A recent textbook (Harwit, 1973) is recommended for reference on fundamental astrophysical questions at the advanced introductory level.
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發(fā)表于 2025-3-22 08:47:47 | 只看該作者
Folgen, Reihen und nichtlineare Gleichungen,esting new data were presented. These include: further measurements of high energy γ-rays from the galaxy by spark chambers on SAS-2 and COS-B, additional observations of Vela-type γ-ray bursts, balloon-borne investigations using cooled Ge(Li) spectrometers searching for γ-ray lines from supernova remnants.
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發(fā)表于 2025-3-22 16:31:13 | 只看該作者
Introduction,rence (Stecker and Trombka, 1973). Stecker (1975) has reviewed the theoretical and experimental work concerned with energetic γ-rays (> 30 MeV). A recent textbook (Harwit, 1973) is recommended for reference on fundamental astrophysical questions at the advanced introductory level.
7#
發(fā)表于 2025-3-22 18:04:28 | 只看該作者
Conclusions,esting new data were presented. These include: further measurements of high energy γ-rays from the galaxy by spark chambers on SAS-2 and COS-B, additional observations of Vela-type γ-ray bursts, balloon-borne investigations using cooled Ge(Li) spectrometers searching for γ-ray lines from supernova remnants.
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,Experimental Considerations for Nuclear γ-Ray Astronomy,, or are being developed for forthcoming experiments, will be reviewed. A recent review by Peterson (1975) gives a discussion of some experimental techniques used in X-ray astronomy and complements some of the discussion here.
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