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Effects of Electromagnetic Waves with LTE and 5G Bandwidth on the Skin Pigmentation In Vitro
(Int J Mol Sci, 2020)
With the rapid growth of wireless communication devices, the influences of electromagnetic fields (EMF) on human health are gathering increasing attention. Since the skin is the largest organ of the body and is located at ...
Non-LTE Monte Carlo radiative transfer. II. Nonisothermal solutions for viscous Keplerian disks
(UNIV CHICAGO PRESS, 2008)
We discuss the basic hydrodynamics that determines the density structure of the disks around hot stars. Observational evidence supports the idea that these disks are Keplerian (rotationally supported) gaseous disks. A ...
Super-luminous type II supernovae powered by magnetars
(EDP Sciences, 2018-05-15)
Magnetar power is believed to be at the origin of numerous super-luminous supernovae (SNe) of Type Ic, arising from compact, hydrogen-deficient, Wolf-Rayet type stars. Here, we investigate the properties that magnetar power ...
DYNAMICAL EVOLUTION OF VISCOUS DISKS AROUND Be STARS. I. PHOTOMETRY
(IOP PUBLISHING LTDBRISTOL, 2012)
Be stars possess gaseous circumstellar disks that modify in many ways the spectrum of the central B star. Furthermore, they exhibit variability at several timescales and for a large number of observables. Putting the pieces ...
Cyanoacetylene in the outflow/hot molecular core G331.512-0.103
(Wiley Blackwell Publishing, Inc, 2019-07)
Using APEX-1 and APEX-2 observations, we have detected and studied the rotational lines of the HC3N molecule (cyanoacetylene) in the powerful outflow/hot molecular core G331.512-0.103. We identified thirty-one rotational ...
Dynamical evolution of viscous disks around Be stars. II. Polarimetry
(American Astronomical SocietyChicago, 2014)
Be stars exhibit variability for a great number of observables. Putting the pieces of the disk dynamics together is not
an easy task and requires arduous modeling before achieving a good fit to the observational data. In ...
Mapping the 13CO/C18O abundance ratio in the massive star-forming region G29.96-0.02
(EDP Sciences, 2018-09)
Aims. Estimating molecular abundances ratios from directly measuring the emission of the molecules toward a variety of interstellar environments is indeed very useful to advance our understanding of the chemical evolution ...