1995
DOI: 10.2172/1033314
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Heat Exchanger Support Bracket Design Calculations

Abstract: Upper horiz. member {4 11 x 8" X 114" wall rect. tubing} 1.1 ksi, tensile 2.2 ksi, shear 9.6 ksi, bending 27 ksi, tensile 18.4 ksi, shear 30.4 ksi, bending 0.357 Vertical member, CASE II {4" x 8" x 114"wall rect. tubing} 1.2 ksi, compressive 2.0 ksi, shear 3.4 ksi, bending 27 ksi, tensile 18.4 kSi, shear 30.4 ksi, bending 0.155 Vertical member, CASE I {411 x 8" x 114" wall rect. tubing} 2.0 ksi, shear 8.7 ksi, bending 18.4 ksi, shear 30.4 ksi, bending not applicable Lower horiz. member {411 x 8" X 1/411 wall r… Show more

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“…We nd E(V{I) = 0.65. This result is in good agreement with the HST photometry of Baade's Window by Holtzman et al (1993){using the new abundance estimates by McWilliam & Rich (1994), as well as with the recent result from W UMa systems by Rucinski (1995). Next, we use as most reliable the direct temperature calibration of V{K photometry from lunar-occultation angular-diameters of eld giants by Ridgway et al (1980) and from Michelson interferometry by Di Benedetto & Rabbia (1987) and Mozurkewich et al (1991).…”
Section: Giants In the Bulgesupporting
confidence: 86%
“…We nd E(V{I) = 0.65. This result is in good agreement with the HST photometry of Baade's Window by Holtzman et al (1993){using the new abundance estimates by McWilliam & Rich (1994), as well as with the recent result from W UMa systems by Rucinski (1995). Next, we use as most reliable the direct temperature calibration of V{K photometry from lunar-occultation angular-diameters of eld giants by Ridgway et al (1980) and from Michelson interferometry by Di Benedetto & Rabbia (1987) and Mozurkewich et al (1991).…”
Section: Giants In the Bulgesupporting
confidence: 86%