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A Young White Dwarf with an Infrared Excess
(IOP Publishing, 2015)
Using observations of Spitzer/IRAC, we report the serendipitous discovery of excess infrared emission from a single white dwarf PG 0010+280. At a temperature of 27,220 K and a cooling age of 16 Myr, it is the hottest and ...
Bright 30 Thz Impulsive Solar Bursts
(AMER GEOPHYSICAL UNIONWASHINGTON, 2015)
When a Red–NIR-Emissive Cs2[Mo6Br14] Interacts with an Active Diureasil–PEO Matrix: Design of Tunable and White-Light-Emitting Hybrid Material
(2019-12-02)
Hybrid materials that combine diureasil matrices and octahedral molybdenum clusters have been synthesized to design lead-, cadmium- and rare-earth-free emitters for lighting or optoelectronic applications. This association ...
Study on suppression of otoacoustic emissions: lateral domain
(Assoc Brasileira Otorrinolaringologia & Cirurgia Cervicofacial, 2011-09-01)
A pon stimulation by contralateral, ipsilateral or bilateral noise, the medial olivocochlear efferent tract changes the amplitude of otoacoustic emissions relative to the tested ear, reducing or removing it; this resulted ...
Eco-friendly polydimethylsiloxane-based self-supporting film containing europium-polyoxometalate: A flexible luminescent material for white light generation
(Elsevier B.V., 2018-09-01)
Lanthanide (Ln(3+))-doped suitable matrices exhibit unique luminescent properties which are important for applications in optoelectronic devices. Most of the Ln(3+)-based luminescent materials are, however, prepared in ...
White light emitting devices by doping polyfluorene with two red emitters
(Elsevier Science SaLausanneSuíça, 2013)
Magnetic fields in close white dwarf binaries
(Universidad de Valparaíso, 2020-09)
White dwarfs are the degenerate remnants of stars that are born with initial masses 8 − 10 Mο (e.g., Smartt et al. 2009 [63], Cummings et al.2019 [16]). Whereas the possibility that some of these stellar remnants possess ...
Constraining the neutrino magnetic dipole moment from white dwarf pulsations
(Iop Publishing, 2014-08)
Pulsating white dwarf stars can be used as astrophysical laboratories to constrain the properties of weakly interacting particles. Comparing the cooling rates of these stars with the expected values from theoretical models ...
White dwarf stars
(Asociación Argentina de Astronomía, 2009)
White dwarfs are the most common end-product of stellarevolution, and as such contain valuable information about the evolutionof individual stars as well as about the star formation history andsubsequent evolution in our ...
Polyfluorene based blends for white light emission
(Elsevier Science BvAmsterdamHolanda, 2011)