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Planck early results. XX. New light on anomalous microwave emission from spinning dust grains
(EDP SCIENCES S A, 2011-12)
Anomalous microwave emission (AME) has been observed by numerous experiments in the frequency range similar to 10-60 GHz. Using Planck maps and multi-frequency ancillary data, we have constructed spectra for two known AME ...
Planck early results. XX. New light on anomalous microwave emission from spinning dust grains
(2011)
Anomalous microwave emission (AME) has been observed by numerous experiments in the frequency range ~10–60 GHz. Using Planck maps and multi-frequency ancillary data, we have constructed spectra for two known AME regions: ...
Enhanced positive and negative exchange bias in FeF2/Ni with dusted interfaces
(American Institute of Physics, 2020)
An enhanced exchange bias was found in FeF2/Ni interfaces by inserting dusting of Pd and Cu atoms. We have used an ultrathin wedge to investigate systematically the effect of a discontinuous nonmagnetic spacer between the ...
Spitzer characterization of dust in an anomalous emission region: the Perseus cloud
(2011)
Anomalous microwave emission is known to exist in the Perseus cloud. One of the most promising candidates to explain this excess of emission is electric dipole radiation from rapidly rotating very small dust grains, commonly ...
Resolved observations at 31 GHz of spinning dust emissivity variations in ρ Oph
(Oxford University Press, 2020-05-14)
The ρ Oph molecular cloud is one of the best examples of spinning dust emission, first detected by the cosmic background imager (CBI). Here, we present 4.5 arcmin observations with CBI 2 that confirm 31 GHz emission from ...
Resolved observations at 31 GHz of spinning dust emissivity variations in rho Oph
(Oxford University Press, 2020)
The rho Oph molecular cloud is one of the best examples of spinning dust emission, first detected by the cosmic background imager (CBI). Here, we present 4.5 arcmin observations with CBI 2 that confirm 31 GHz emission from ...
The State-of-Play of anomalous microwave eission (AME) research
(Elsevier, 2018)
Anomalous Microwave Emission (AME) is a component of diffuse Galactic radiation observed at frequencies in the range approximate to 10-60 GHz. AME was first detected in 1996 and recognised as an additional component of ...
Planck intermediate results. XV. A study of anomalous microwave emission in Galactic clouds
(European Southern Observatory., 2014-05-20)
Anomalous microwave emission (AME) is believed to be due to electric dipole radiation from small spinning dust grains. The aim of this paper is
a statistical study of the basic properties of AME regions and the environment ...
Modelling the spinning dust emission from LDN1780
(Oxford University Press, 2020)
We study the anomalous microwave emission (AME) in the Lynds Dark Nebula (LDN) 1780 on two angular scales. With publicly available data at an angular resolution of 1 degrees, we studied the spectral energy distribution of ...