By P.L. Biermann, G. Börner, M. Camenzind, K.J. Fricke, B. Fuchs, R. Genzel, W.K. Huchtmeier, H. Jahreiß, A.R. Just, B.F. Madore, H. Netzer, H. Schwan, B.. Wiebel-Sooth, A. Witzel, Zimmermann
Astronomy and Astrophysics have been first handled in quantity III of the sixth variation of Landolt-Börnstein in 1952, then in volumes VI/1 and VI/2 of the hot sequence, 1965 and 1981/82 respectively. the current quantity VI/3 is an extra supplementation of quantity VI/1. The decimal class scheme of the 1st complement volumes, VI/2, has been maintained, fields with no major new advancements are truly indicated. A synoptic checklist of contents over all 3 volumes presents a good evaluate for the consumer in addition to a entire Index within the impending final subvolume of VI/3.
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Instit. Ser. Vol. 487. Dordrecht: Kluwer (1996). : in [96G1], p. 43. : in [96G1], p. 1. : in [96G1], p. 133. 1 General references List of LB VI/2c subsect. 1. p. 126, updated. F. : Molecular Astrophysics - State of the Art and Future Directions. Dordrecht: Reidel (1985). : Molecular Collisions in the Interstellar Medium. Cambridge: Univ. Press (1990). A. ): Interstellar Processes, Proceed. Symp. on Interstellar Processes, Astrophys. Space Sci. Libr. Vol. 134. Dordrecht: Reidel (1987). A. ): Rate Coefficients in Astrochemistry.
P. 5 18 30 SiC Silicates MgS ? A detailed spectroscopic discussion of observed emission bands is given by Allamandola et al. [89A1]. Dust-related visual continuous emission The Extended Red Emission band, usually between about 6000 and 8000 Å, takes the form of a broad band peaking near 6700 Å with about 1200 Å FWHM [89W] and can be fitted well with the measured band-gap emission from hydrogenated amorphous carbon [90W]. 4 Grain models Table 3. Materials suggested as constituents of interstellar grains, in addition to the materials listed in LB VI/2c subsect.
L. 75…2 m2) scintillator stations, ionization calorimeter, several gas discharge hodoscopes. l. Energy range: 300 TeV…70 PeV Operating: since 1996 Technique: 13 Cherenkov counters. Landolt-Börnstein New Series VI/3C Ref. p. l. Energy range: 300 TeV…30 PeV Technique: 13 open Cherenkov counters. l. 25 m2) scintillator stations, 6 × (20 m2) muon detectors, 53 Cherenkov detectors, 7 Cherenkov pulse form detectors, 10 radio antennas (32 MHz). 5 The main elements in the TeV range Plotting the data of individual nuclei as provided by the direct experiments so far, without using further adjustments, shows in general a fair correspondence in overlapping energy ranges.