Accelerated glacier mass loss in the southeastern Tibetan Plateau since the 1970s
The southeastern Tibetan Plateau (SETP) is a region in High Mountain Asia with the most serious glacier mass loss. However, long-term and large regional-scale studies that estimate glacier mass balance in this area remain limited.
Lan-Hua Luo +3 more
doaj +1 more source
Global hot-star wind models for stars from Magellanic Clouds
We provide mass-loss rate predictions for O stars from Large and Small Magellanic Clouds. We calculate global (unified, hydrodynamic) model atmospheres of main sequence, giant, and supergiant stars for chemical composition corresponding to Magellanic ...
Krticka, Jiri, Kubat, Jiri
core +1 more source
Radio emission from the massive stars in the Galactic Super Star Cluster Westerlund 1 [PDF]
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
Stellar coronal mass ejections – I. Estimating occurrence frequencies and mass-loss rates [PDF]
18 pages, 8 figures, 1 table, accepted to ...
Odert, P. +3 more
openaire +2 more sources
Rate of Mass Loss Across the Instability Threshold for Thwaites Glacier Determines Rate of Mass Loss for Entire Basin [PDF]
AbstractRapid change now underway on Thwaites Glacier (TG) raises concern that a threshold for unstoppable grounding line retreat has been or is about to be crossed. We use a high‐resolution ice sheet model to examine the mechanics of TG self‐sustained retreat by nudging the grounding line just past the point of instability.
M. S. Waibel +3 more
openaire +3 more sources
Constraints on porosity and mass loss in O-star winds from modeling of X-ray emission line profile shapes [PDF]
We fit X-ray emission line profiles in high resolution XMM-Newton and Chandra grating spectra of the early O supergiant Zeta Pup with models that include the effects of porosity in the stellar wind.
Cohen, David H. +3 more
core +3 more sources
We provide hot star wind models with radiative force calculated using the solution of comoving frame (CMF) radiative transfer equation. The wind models are calculated for the first stars, O stars, and the central stars of planetary nebulae.
Abbott +73 more
core +1 more source
Prediction Method of Steel Corrosion Rate Based on the Helix Distributed Sensor
Corrosion of steel bars is of great significance for safety and service life of reinforced concrete structures. This work develops a prediction method for steel corrosion mass loss rate before the crack of concrete structure based on a spiral distributed
Jian-Zhi Li, Yi-Yao Zhao, Jun-Jie Wang
doaj +1 more source
Study on Corrosion Resistance of Basalt Fiber in Guizhou
This is an article in the field of ceramics and composites. In order to explore the resistance of basalt fiber to acid and alkali corrosion, basalt fiber with or without wetting agent was soaked in 3 mol/L sulfuric acid solution and sodium hydroxide ...
Man CHEN +5 more
doaj +1 more source
Prevalence and Trajectory of Household Material Hardship Among Children With Advanced Cancer
ABSTRACT Background/Objectives Families of children with advanced cancer living in poverty experience inferior outcomes including poor parent mental health and worse child quality of life. Household material hardship (HMH: food, housing, transportation, and/or utility insecurity) is a modifiable poverty exposure—and potential intervention target—that ...
Sarah Wright +13 more
wiley +1 more source

