Influence of Simultaneous Mechanical and Electrical Straining on Conventional Thick-Film Resistors

Stanimirovic, Z.; Jevtic, M.M.; Stanimirovic, I.

doi:10.1109/icmel.2006.1651035

Cited by 1 publication

(2 citation statements)

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“…We would now like to draw attention to numerous HI clouds found recently in the interface region between the disk and the halo of our Galaxy (Lockman 2002;Stil et al 2005;Stanimirović et al 2006). These clouds are small, 5-20 pc in size, cold (< 400 to 1000 K), and often kinematically follow the Galactic disk but at a velocity that is offset by 10-20 km s −1 from that of the bulk HI emission.…”

Section: What Happens To Shells At a Very Late Stage Of Their Evolution?mentioning

confidence: 99%

“…Lockman, Pidopryhora, & Shields (2006) found a large plume-like structure which has numerous clouds. Stanimirović et al. (2006) found that clouds are embedded in large filamentary structures and morphologically resemble cold clouds that form in simulations of dynamically triggered instabilities (e.g.…”

Section: What Happens To Shells At a Very Late Stage Of Their Evolution?mentioning

confidence: 99%

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Shells in the Magellanic System

Stanimirović

2006

Proc. IAU

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Abstract. The Magellanic System harbors > 800 expanding shells of neutral hydrogen, providing a unique opportunity for statistical investigations. Most of these shells are surprisingly young, 2-10 Myr old, and correlate poorly with young stellar populations. I summarize what we have learned about shell properties and particularly focus on the puzzling correlation between the shell radius and expansion velocity. In the framework of the standard, adiabatic model for shell evolution this tight correlation suggests a coherent burst of star formation across the whole Magellanic System. However, more than one mechanism for shell formation may be taking place.

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Section: What Happens To Shells At a Very Late Stage Of Their Evolution?mentioning

confidence: 99%

Section: What Happens To Shells At a Very Late Stage Of Their Evolution?mentioning

confidence: 99%