Energy Technology Data Exchange (ETDEWEB)

The effect of partial and total replacement of tungsten by molybdenum on the mechanical technical properties were investigated with the cold work steel 60 WCrV 7 (DIN 1.2550). While maintaining the total quantity of tungsten atoms and/or molybdenum atoms in the steel, no differences occur in the type of the separated carbides. After annealing in the range of the pearlite stage with annealing times of up to 150 h, the carbide phases M/sub 23/C/sub 6/ and MC are, besides alpha iron, also present. In short-time annealed states also M/sub 6/C carbides occur. These are formed during austeniting and remain in the steel as residual carbides in austeniting treatment carried out under normal conditions. Compared with tungsten alloyed steel, there is an increased formation of M/sub 6/C carbides in molybdenum alloyed steels during austeniting. By a long-time annealing treatment in the range of the pearlite stage, the M/sub 6/C carbides are dissolved in ...

International Nuclear Information System (INIS)

We present 14 years of contemporaneous photometric and spectroscopic observations of 28 solar analog stars, taken with the Tennessee State University Automatic Photometric Telescopes at Fairborn Observatory and the Solar-Stellar Spectrograph at Lowell Observatory. These are the best observed and most nearly Sun-like of the targets in our magnitude-limited (V #<=# 7.5) sample. The correlations between luminosity and activity reveal the expected inverse activity-brightness correlations for active stars. Strong direct correlations between activity and brightness are not prevalent for the less active solar age stars, but are precision limited. The Sun does not appear to have unusually low photometric variability when compared with the most Sun-like inactive solar analogs. We present evidence that the activity index R'_H_K is not a good discriminant of Maunder Minimum candidate stars. On the basis of a star that appears to have transitioned from ...

International Nuclear Information System (INIS)

Neutron-hole states in /sup 87/Sr were studied by means of the /sup 88/Sr("3He,#alpha#)/sup 87/Sr reaction at 36 MeV. Angular distribution measurements were carried out from 3"0 to 41"0 (lab) and analyzed with the zero-range distorted-wave Born approximation method. Spectroscopic factors have been determined for about 50 discrete levels in /sup 87/Sr located below 6 MeV excitation energy and for the three lowest isobaric analog states 2p(3/2, 1f(5/2, and 2p(1/2 observed around 11 MeV. Many l = 1 and l = 3 discrete levels are observed in the 3--6 MeV excitation energy range. In addition, a large part of the 1f-2p strength is found to lie in the higher-lying continuum up to 13 MeV (about 10% and 40% for the l = 1 and 3 contributions, respectively). The distribution of the 1f-2p neutron-hole strength is compared to previous data on neighboring nuclei /sup 89/Zr and /sup 91/Mo. In addition, angular distributions for some low-lying high-spin states in /sup 87/Sr are nicely reproduced by ...