Results 61 to 70 of about 1,618,200 (249)

Searching for hot subdwarf stars from the LAMOST spectra. III. classifying the hot subdwarf stars from LAMOST DR4 using deep learning method [PDF]

open access: yes, 2018
Hot subdwarf stars are core He burning stars located at the blue end of the horizontal branch, also known as the extreme horizontal branch. The properties of hot subdwarf stars are important for our understanding of the stellar astrophysics, globular clusters and galaxies.
arxiv   +1 more source

Estimate of the Upper Limit on Hot Plasma Differential Emission Measure (DEM) in Non-Flaring Active Regions and Nanoflare Frequency Based on the Mg XII Spectroheliograph Data from CORONAS-F/SPIRIT [PDF]

open access: yesSolar Physics, 2018, 293:140, 2018
The nanoflare-heating theory predicts steady hot plasma emission in the non-flaring active regions. It is hard to find this emission with conventional non-monochromatic imagers (such as Atmospheric Imaging Assembly or X-Ray Telescope), because their images contain a cool temperature background.
arxiv   +1 more source

Universal Minimum Heat Leak on Low-Temperature Metallic Electrical Leads

open access: yes, 2006
Low-temperature electronic systems require electrical leads which have low electrical resistance to provide bias current I without excessive voltage drop V. But proper cryogenic design also requires high thermal resistance to maintain a minimum heat leak
Kadin, Alan M.
core   +1 more source

Hot ductility and deformation behavior of C-Mn/Nb-microalloyed steel related to cracking during continuous casting [PDF]

open access: yes, 2014
Hot ductility studies have been performed on C-Mn and C-Mn-Nb steels with an approach to simulate the effect of cooling conditions experienced by steel in secondary cooling zone during continuous casting.
Lanjewar, Harishchandra   +3 more
core   +1 more source

X-ray Observations of Complex Temperature Structure in the Cool-core cluster Abell 85

open access: yes, 2014
X-ray observations were used to examine the complex temperature structure of Abell 85, a cool-core galaxy cluster. Temperature features can provide evidence of merging events which shock heat the intracluster gas.
Burns, Jack   +3 more
core   +1 more source

Breakdown of Fermi liquid behavior at the (\pi,\pi)=2k_F spin-density wave quantum-critical point: the case of electron-doped cuprates [PDF]

open access: yes, 2012
Many correlated materials display a quantum critical point between a paramagnetic and a SDW state. The SDW wave vector connects points (hot spots) on opposite sides of the Fermi surface.
A.-M. S. Tremblay   +9 more
core   +2 more sources

Impact of Depression on Activation and Summer Heat Adaptation in Older Adults With Cardiovascular Concerns: Empirical Research Quantitative

open access: yesNursing Open
Aim To investigate the effects of depression on patient activation and summer heat adaptation, considering important contributory factors in older adults with increased cardiovascular health concerns on extremely hot days.
Yuli Zang   +3 more
doaj   +1 more source

Performance enhancement of air conditioner in hot climate by condenser cooling with cool air generated by direct evaporative cooling

open access: yesCase Studies in Thermal Engineering, 2021
This research studied the direct evaporative cooling technique for generating cool air in hot–dry and hot–humid climates. For direct evaporative cooling, three parameters affected the air temperature: feedwater temperature, wet-bulb temperature, and mass
Wichakan Ketwong   +2 more
doaj  

Predicting the Temperature Field of Hot Dry Rocks by the Seismic Inversion Method

open access: yesEnergies, 2023
Hot dry rocks, as clean and abundant sources of new energy, are crucial in the restructuring of energy. Predicting the temperature field of hot dry rocks is of great significance for trapping the target areas of hot dry rocks.
Hongjie Peng, Jingtao Zhao, Rui Cui
doaj   +1 more source

Hot electron cooling in Dirac semimetal Cd$_3$As$_2$ due to polar optical phonons

open access: yes, 2018
A theory of hot electron cooling power due to polar optical phonons $P_{\rm op}$ is developed in three-dimensional Dirac semimetal($3$DDS) Cd$_3$As$_2$ taking account of hot phonon effect.
Biswas, Tutul, Kubakaddi, Shrishail S.
core   +1 more source

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