Results 31 to 40 of about 4,471,573 (294)

Mass-Losing Semiregular Variable Stars in Baade's Windows [PDF]

open access: yes, 2001
By cross-correlating the results of two recent large-scale surveys, the general properties of a well defined sample of semi-regular variable stars have been determined.
A. B. Tomaney   +61 more
core   +3 more sources

The polishing methods for large area CVD diamond wafer

open access: yesFunctional Diamond, 2023
The mainstream polishing methods were reviewed in light of polycrystalline CVD diamond wafer with large area. The principles, equipment, and processes of the mainstream polishing methods were reviewed, and the processing characteristics of these methods ...
Haochen Zhang   +7 more
doaj   +1 more source

Atmospheric Mass Loss During Planet Formation: The Importance of Planetesimal Impacts [PDF]

open access: yes, 2014
We quantify the atmospheric mass loss during planet formation by examining the contributions to atmospheric loss from both giant impacts and planetesimal accretion. Giant impacts cause global motion of the ground.
Sari, Re'em   +2 more
core   +2 more sources

Initial Stages of AZ31B Magnesium Alloy Degradation in Ringer’s Solution: Interpretation of EIS, Mass Loss, Hydrogen Evolution Data and Scanning Electron Microscopy Observations

open access: yesMetals, 2018
The initial stages of corrosion of AZ31B magnesium alloy, immersed in Ringer’s solution at 37 °C body temperature for four days, have been evaluated by independent gravimetric and chemical methods and through electrochemical impedance ...
Lucien Veleva   +2 more
doaj   +1 more source

Mass loss and stellar superwinds [PDF]

open access: yesPhilosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences, 2017
Mass loss bridges the gap between massive stars and supernovae (SNe) in two major ways: (i) theoretically, it is the amount of mass lost that determines the mass of the star prior to explosion and (ii) observations of the circumstellar material around SNe may teach us the type of progenitor that made the SN.
openaire   +3 more sources

Conservation of minimally processed green pepper conditioned in different plastic packages

open access: yesPesquisa Agropecuária Tropical, 2012
Minimal processing of vegetables adds value to the final product for increasing its convenience and reducing the time to prepare meals. This study aimed to evaluate the conservation of minimally processed green peppers 'Konan R', sliced and conditioned ...
Brígida Monteiro Vilas Boas   +4 more
doaj   +1 more source

Cepheid Mass-loss and the Pulsation -- Evolutionary Mass Discrepancy

open access: yes, 2008
I investigate the discrepancy between the evolution and pulsation masses for Cepheid variables. A number of recent works have proposed that non-canonical mass-loss can account for the mass discrepancy.
Andreasen G. K.   +19 more
core   +1 more source

Biodegradability and Cavitation Erosion Behavior of Some Zinc Alloys from the System ZnCuMg

open access: yesMetals
This paper presents experimental results regarding the development of new alloys from the binary ZnCu and ternary ZnCuMg systems. The alloys had controlled chemical compositions and were annealed at 300 °C and 400 °C, with holding times of 5 h and 10 h ...
Brandusa Ghiban   +7 more
doaj   +1 more source

Radio emission from the massive stars in the Galactic Super Star Cluster Westerlund 1 [PDF]

open access: yes, 2009
Current mass-loss rate estimates imply that main sequence winds are not sufficient to strip away the H-rich envelope to yield Wolf-Rayet (WR) stars. The rich transitional population of Westerlund 1 (Wd 1) provides an ideal laboratory to observe mass-loss
Chapman, J. M.   +4 more
core   +3 more sources

Mass-Loss from Spinning Stars [PDF]

open access: yesHighlights of Astronomy, 1980
AbstractThe effects of mass-loss and angular momentum loss on the evolution of massive stars are discussed bringing out the main results as well as the limitations of recent studies. It is pointed out that an acceptable theory of stellar winds in early as well as late type stars is needed as well as a satisfactory assessment of a number of ...
openaire   +1 more source

Home - About - Disclaimer - Privacy