# Solucionario Optaciano Vasquez G

Solucionario Optaciano Vasquez G

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abstract: ‘We present results from a new study with photometry of the galactic Cepheid $\eta$ Aql and its companion $\beta$ Cepheid $\alpha$ Cep. We have supplemented the data with 2MASS NIR photometry. With the aid of 9,250 photographic plates we were able to reduce the errors in the light curves and analyze the data in the usual way to obtain periods and amplitude ratios. We find that the amplitude ratio is not only constant but is 0.46$\pm$0.02. The new periods are $P_\eta = 3.568\pm0.001$ and $P_\beta = 5.591\pm0.001$, which is in good agreement with the previously published periods. The long term behaviour of these two stars is characteristic of resonance effects.’
author:
– |
P. K. Seethiraman$^1$[^1], A. S. Raveendran$^2$, M. A. P. Boyd$^3$, and I. J. J. Eyers$^1$\
$^1$Department of Physics & Astronomy, University of Western Ontario, London, N6A 3K7, Ontario, Canada\
$^2$School of Mathematics & Physics, Keele University, Keele, Staffordshire, ST5 5BG, UK\
$^3$Department of Physics, University of Calgary, Calgary, Alberta, Canada, T2N 1N4
date: ‘Accepted –. Received –; in original form –’
title: The Period and Ratio of $\eta$ Aql and $\alpha$ Cep

stars: variables – techniques: photometric – stars: $\eta$ Aquilae – stars: $\beta$ Cephei

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Introduction {#

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Solucionario Optaciano Vasquez G
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ROBERT DE SILVA,
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you can download full Software Review from the given link. You can get best RSS Feed from the link.The present invention relates to a sensor device that is used to detect the amount of a fluid flowing through a vent line in an exhaust pipe, etc.
A previously known sensor device for detecting the amount of fluid flowing through a vent line of an exhaust pipe, etc., as disclosed in Japanese Examined Utility Model Publication No. H2-13565, has a magnetic detecting portion formed by winding a magnetic flux generating element such as an amorphous magnetic alloy ribbon so as to face a sensor case formed with a detecting passage. This conventional sensor device detects variations in magnetic flux density generated by the magnetic flux generating element to thereby detect the amount of fluid flowing through the detecting passage.
In this conventional sensor device, however, since the magnetic detecting portion is provided in the sensor case, there is a possibility that the temperature of the magnetic detecting portion is increased by heat emitted from the part of the engine, especially in a case where the sensor device is installed in the vicinity of the exhaust pipe of a vehicle engine. In order to minimize a temperature rise of the magnetic detecting portion caused by heat emission from the engine, it is necessary to set the distance between the part of the engine generating heat and the magnetic detecting portion so as to be as large as possible. As a result, the diameter of the detecting passage for detecting the amount of fluid flowing therethrough tends to be enlarged to such an extent that an error in fluid detection is caused by a difference in amount of fluid that flows through a vent line of the exhaust pipe.
On the other hand, there is an increasing demand for miniaturizing the exhaust pipe. Since the vent line is located in the vicinity of a highly temperature

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