Detections of Massive Stars in the Cluster MCM2005b77, in the Star-forming Regions GRS G331.34−00.36 (S62) and GRS G337.92−00.48 (S36) [PDF]
, 2018 Maria Messineo +4 more
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Using the Photostationary State of Arylazopyrazoles to Control Phase Transitions of Liquid Crystals
Advanced Functional Materials, EarlyView.A series of new arylazopyrazole photoswitches is designed as dopants for liquid crystalline materials. Unprecedented, the distribution of photoisomers at the photostationary state upon irradiation with light of specific wavelengths (365, 460, 520 nm) is used to control the liquid crystalline phase transitions under isothermal conditions, including ...
Tobias Thiele +3 more
wiley +1 more source
Stellar Evolution Through the Red Supergiant Phase
GalaxiesMassive stars less massive than ∼30 M⊙ evolve into a red supergiant after the main sequence. Given a standard IMF, this means about 80% of all single massive stars will experience this phase.
Sylvia Ekström, Cyril Georgy
doaj +1 more source
Luminous blue variables and the fates of very massive stars. [PDF]
Philos Trans A Math Phys Eng Sci, 2017 Smith N.
europepmc +1 more source
Peculiar Intrinsic Parameters of Massive Stars as a Result of an Early Phase of Homogeneous Evolution [PDF]
, 1993 K. P. Simon
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Electron–Matter Interactions During Electron Beam Nanopatterning
Advanced Functional Materials, EarlyView.This article reviews the electron–matter interactions important to nanopatterning with electron beam lithography (EBL). Electron–matter interactions, including secondary electron generation routes, polymer radiolysis, and electron beam induced charging, are discussed.
Camila Faccini de Lima +2 more
wiley +1 more source
Hyperaccretion-driven Relativistic Jets from Massive Collapsars in Active Galactic Nucleus Disks
The Astrophysical JournalThe observable characteristics of gamma-ray bursts embedded in the accretion disk of active galactic nuclei (AGNs) are mainly determined by the jet propagation within the disk.
Yun-Feng Wei, Tong Liu, Bao-Quan Huang
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The evolution of massive stars: bridging the gap in the Local Group. [PDF]
Philos Trans A Math Phys Eng Sci, 2017 Massey P, Neugent KF, Levesque EM.
europepmc +1 more source
Spectroscopic variability of massive pre-main-sequence stars in M17 [PDF]
, 2023 Annelotte Derkink +6 more
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