Determination of percolation probability from the use of a concentration gradient

The MICs of streptomycin for Salmonella isolates from swine and poultry were determined by a micro-broth dilution technique. The Salmonella isolates were recovered from the lymph nodes and cecal contents of market-age swine and from the cecal contents of poultry at the time of slaughter and were found by disk diffusion to be resistant to 10 μg of streptomycin. MIC testing was carried out with the Sensititre susceptibility system for streptomycin, which uses a microwell concentration gradient of 16 to 800 μg/ml. Results indicated that >80% of the swine isolates had MICs of ≤64 μg/ml, while 51% of poultry isolates exhibited MICs of ≥128 μg/ml. The highest MICs observed in swine and poultry were 256 and 800 μg/ml, respectively. Replicate tests performed on 12 of the isolates chosen at random indicated a 100% correlation between runs. Advantages of this system include easily read results and precoated wells. Disadvantages include the cost and the inability to test concentrations of streptomycin other than those in the wells. We found this micro-broth dilution commercial test kit to provide a relatively quick and easy testing procedure for the determination of streptomycin resistance in Salmonella.

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THE EFFECT OF HYDROGEN ION CONCENTRATION UPON THE INDUCTION OF POLARITY IN FUCUS EGGS

The Journal of General Physiology ◽

10.1085/jgp.21.1.57 ◽

1937 ◽

Vol 21 (1) ◽

pp. 57-70 ◽

Cited By ~ 11

Author(s):

D. M. Whitaker ◽

E. W. Lowrance

Keyword(s):

Oxygen Tension ◽

Concentration Gradient ◽

Sea Water ◽

Capillary Tube ◽

Hydrogen Ion ◽

Developmental Pattern ◽

Ion Concentration ◽

Hydrogen Ion Concentration ◽

Ph Values

1. When a Fucus egg develops near one end in a close fitting capillary tube of pyrex glass or silica (quartz), diffusion of substances passing to and from the egg is more impeded on the side of the egg toward the far end of the tube. 2. The egg therefore develops in a gradient of its own diffusion products, and of oxygen tension. 3. More than 600 eggs have been reared, each near one end in a capillary, in sea water at various regulated and measured pH values. 4. When the medium, which is initially homogeneous inside and outside the capillary, is initially at pH 6.5 to 7.6, nearly all of the eggs develop rhizoid protuberances on the sides of the eggs toward the far ends of the capillaries. This is on the sides of the eggs where the concentration of substances diffusing from the eggs is greatest. 5. The polarity and developmental pattern of the egg is thus determined either by a concentration gradient of products diffusing from it, or by a gradient of oxygen tension. The former interpretation is favored. 6. This is regarded as an extension of earlier observations that rhizoid protuberances form on the sides of two neighboring eggs in the direction of the neighbor if the sea water is acidified. 7. It appears hardly possible that a mitogenetic effect could be responsible for the response of an egg to its own diffusion gradients. 8. When the medium is made more basic, the percentage of the eggs which form rhizoid protuberances toward the far end of the tube decreases to about 20 or 25 per cent between pH 8.1 and 8.6. The response of the egg to the gradients which it produces is thus statistically reversed. The determination of the polarity of the eggs by the diffusion gradients does not become as complete in alkalinized as in acidified sea water. 9. When the pH of the sea water is elevated to 9.1 or 9.2, salts precipitate out. The type of development is altered and the control of the diffusion gradients over the polarity of the eggs decreases.

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Galactic orbits of stars

Symposium - International Astronomical Union ◽

10.1017/s0074180900105340 ◽

1966 ◽

Vol 25 ◽

pp. 93-97

Author(s):

Richard Woolley

Keyword(s):

Globular Cluster ◽

Potential Field ◽

High Velocity ◽

Velocity Vector ◽

Variable Stars ◽

The Sun ◽

Proper Motions ◽

Rr Lyrae ◽

The Galaxy

It is now possible to determine proper motions of high-velocity objects in such a way as to obtain with some accuracy the velocity vector relevant to the Sun. If a potential field of the Galaxy is assumed, one can compute an actual orbit. A determination of the velocity of the globular clusterωCentauri has recently been completed at Greenwich, and it is found that the orbit is strongly retrograde in the Galaxy. Similar calculations may be made, though with less certainty, in the case of RR Lyrae variable stars.

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Distance to SN 1987A and the LMC

Symposium - International Astronomical Union ◽

10.1017/s0074180900118959 ◽

1999 ◽

Vol 190 ◽

pp. 549-554

Author(s):

Nino Panagia

Keyword(s):

Angular Size ◽

Large Magellanic Cloud ◽

Magellanic Cloud ◽

Light Curves ◽

Distance Modulus ◽

Absolute Size ◽

Sn 1987A

Using the new reductions of the IUE light curves by Sonneborn et al. (1997) and an extensive set of HST images of SN 1987A we have repeated and improved Panagia et al. (1991) analysis to obtain a better determination of the distance to the supernova. In this way we have derived an absolute size of the ringRabs= (6.23 ± 0.08) x 1017cm and an angular sizeR″ = 808 ± 17 mas, which give a distance to the supernovad(SN1987A) = 51.4 ± 1.2 kpc and a distance modulusm–M(SN1987A) = 18.55 ± 0.05. Allowing for a displacement of SN 1987A position relative to the LMC center, the distance to the barycenter of the Large Magellanic Cloud is also estimated to bed(LMC) = 52.0±1.3 kpc, which corresponds to a distance modulus ofm–M(LMC) = 18.58±0.05.

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