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1.
BOOK
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Distance determination of variable X-ray sources (1973)
Garching bei München
MPE-Report
Call number: SR 90.1026(82)
Series Statement: [Max-Planck-Institut für Physik und Astrophysik, Institut für Extraterrestrische Physik 82]
Type of Medium: Series available for loan
Pages: 20 S.
Location: Magazine - must be ordered
Branch Library: GFZ Library
2.
BOOK
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Diffuse cosmic and Atmospheric MeV gamma radiation from balloon observations (1977)
Garching bei München
MPE-Report
Call number: SR 90.1026(133)
Series Statement: [Max-Planck-Institut für Physik und Astrophysik, Institut für Extraterrestrische Physik 133]
Type of Medium: Series available for loan
Pages: 35 S.
Location: Magazine - must be ordered
Branch Library: GFZ Library
3.
BOOK
get availability status
Energy spectrum and evidence for Extragalactic Origin of diffuse Gamma-Radiation in the MeV-Range (1974)
Garching bei München
MPE-Report
Call number: SR 90.1026(95)
Series Statement: [Max-Planck-Institut für Physik und Astrophysik, Institut für Extraterrestrische Physik 95]
Type of Medium: Series available for loan
Pages: 12 S.
Location: Magazine - must be ordered
Branch Library: GFZ Library
4.
BOOK
get availability status
A telescope for soft gamma ray astronomy (1972)
München
MPE-Report
Call number: SR 90.1026(74)
Series Statement: [Max-Planck-Institut für Physik und Astrophysik, Institut für Extraterrestrische Physik 74]
Type of Medium: Series available for loan
Pages: 24 S.
Location: Magazine - must be ordered
Branch Library: GFZ Library
5.
Paper (German National Licenses)
Gamma ray astronomy and search for antimatter in the universe (1989)
Springer
Hyperfine interactions 44 (1989), S. 85-96 
ISSN: 1572-9540
Source: Springer Online Journal Archives 1860-2000
Kategorien: Physics
Notes: Abstract Gamma ray astronomy provides a powerful tool for searching antimatter in the universe; it probably provides the only means to determine, if the universe has baryon symmetry. Presently existing gamma-ray observations can be interpreted without postulating the existence of antimatter. However, the measurements are not precise enough to definitely exclude the possibility of its existence. The search for antimatter belongs to one of the main scientific objectives of the Gamma Ray Observatory GRO of NASA, which will be launched in 1990 by the Space Shuttle.
Type of Medium: Electronic Resource
6.
Paper (German National Licenses)
Galaktische Gamma-Astronomie (1982)
Springer
Naturwissenschaften 69 (1982), S. 212-219 
ISSN: 1432-1904
Source: Springer Online Journal Archives 1860-2000
Kategorien: Biology , Chemistry and Pharmacology , Natural Sciences in General
Notes: Abstract During the last decade the exploration of the sky in the light of gamma rays has begun by means of satellite- and balloon-borne instruments. Like in other ranges of the electromagnetic spectrum the Milky Way clearly stands out against the rest of the sphere. Part of the galactic γ-ray emission is due to discrete sources, part is diffuse in origin and is produced in interstellar space. Some of the discrete γ-ray sources are radio pulsars, the nature of the other sources is still unknown. The intensity distribution of the diffuse galactic γ-ray component is consistent with a decrease of the cosmic-ray intensity towards the outer part of the galaxy. The identification of the cosmic-ray sources will be one of the main objectives of the next generation of γ-ray telescopes.
Type of Medium: Electronic Resource
7.
Paper (German National Licenses)
Wie aussichtsreich ist die Suche nach Gamma-Pulsaren? (1985)
Springer
Naturwissenschaften 72 (1985), S. 133-138 
ISSN: 1432-1904
Source: Springer Online Journal Archives 1860-2000
Kategorien: Biology , Chemistry and Pharmacology , Natural Sciences in General
Type of Medium: Electronic Resource
8.
Paper (German National Licenses)
Die diffuse kosmische Gamma-Strahlung (1974)
Springer
Naturwissenschaften 61 (1974), S. 250-256 
ISSN: 1432-1904
Source: Springer Online Journal Archives 1860-2000
Kategorien: Biology , Chemistry and Pharmacology , Natural Sciences in General
Type of Medium: Electronic Resource
9.
Paper (German National Licenses)
Origin of the diffuse galactic gamma-ray emission at low and medium gamma-ray energies (1983)
Springer
Space science reviews 36 (1983), S. 249-266 
ISSN: 1572-9672
Source: Springer Online Journal Archives 1860-2000
Kategorien: Physics
Notes: Abstract Recently the galactic plane has been observed in the low and medium energy gamma-ray range in the directions towards the center and anticenter. Spectral measurements are now available at those energies, where the contribution from π°-decay gamma rays can be neglected. The high MeV-fluxes observed in both parts of the Galaxy are an indication of either a strong electron induced component or a high contribution from unresolved sources. Several interstellar cosmic-ray electron spectra have been used to calculate the contribution from electron bremsstrahlung and inverse Compton collisions with optical, infrared and 2.7 K black-body photons. From these calculations restrictions on the interstellar electron spectrum are derived.
Type of Medium: Electronic Resource
10.
Paper (German National Licenses)
ISSN: 1572-9672
Source: Springer Online Journal Archives 1860-2000
Kategorien: Physics
Notes: Abstract The GRASP mission Gamma-Ray Astronomy with Spectroscopy and Positioning addresses the scientific goals of fine spectroscopy with imaging and accurate positioning of gamma-ray sources, an unexplored area within gamma-ray astronomy. The assessment of GRASP as a future space astronomy mission in the mid-1990s has led to the design of the instrument outlined in this article. Thus GRASP is a third generation gamma-ray telescope and is designed to operate as a high quality spectral imager in the mid-1990s, when, following the GRO, SIGMA, and GAMMA-1 missions, there will be requirement for a more sophisticated instrument to maintain the momentum of advance in gamma-ray astronomy. The telescope will be capable of locating point sources with a precision of typically 1 arc min, whilst making a fine spectral analysis (E/ΔE ∼ 1000) of any gamma-ray line features. The high sensitivity of this instrument and the long (> 2 year) lifetime of the mission will enable a large number (∼ 1000) of astronomical objects to be studied. The GRASP mission has the potential to move gamma-ray astronomy from an era of basic exploration to one in which detailed and novel measurements can be used to gain a better understanding of many astrophysical problems.
Type of Medium: Electronic Resource