ACA Band 7 observations of W28F reveal shocked clumps with nH2 ~ (1-3)×10^5 cm^-3, Tgas ~50-170 K showing density-temperature anti-correlation, pressure balance with hot plasma, E/A-CH3OH ratio >0.9, and CH3OH/SiO spatial-spectral segregation attributed to slow vs fast shocks.
Title resolution pending
2 Pith papers cite this work, alongside 27 external citations. Polarity classification is still indexing.
2
Pith papers citing it
27
external citations · OpenAlex
fields
astro-ph.GA 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
New infrared spectra show reduced water ice and unusually strong aliphatic hydrocarbon absorption towards W44, attributed to shock and cosmic-ray processing in the associated molecular cloud.
citing papers explorer
-
An ACA map of a molecular cloud interacting with supernova remnant W28
ACA Band 7 observations of W28F reveal shocked clumps with nH2 ~ (1-3)×10^5 cm^-3, Tgas ~50-170 K showing density-temperature anti-correlation, pressure balance with hot plasma, E/A-CH3OH ratio >0.9, and CH3OH/SiO spatial-spectral segregation attributed to slow vs fast shocks.
-
Dust Absorption towards Supernova Remnant W44
New infrared spectra show reduced water ice and unusually strong aliphatic hydrocarbon absorption towards W44, attributed to shock and cosmic-ray processing in the associated molecular cloud.