... The positions of the infrared emission bands produced by these minerals are ... important for the identification of emission features in astronomical spectra [ 7 ... the spectra indicate positions of astronomically observed emission bands (after [ 6 ...
... Magnesium-aluminium spinel (MgAl O ) has been considered as a primary condensate in the outflows of oxygen-rich AGB stars and as a potential carrier of the 13 m emission band observed in the spectra of these stars [ 11 ]. ...
... Next: Absorption/emission properties Up: Optical properties of cosmic Previous: Circular polarization: change of . to be given . root 2003-04-09. ...
... Emission of the inhomogeneous plasma: line intensities and element abundances in the gaseous nebulae with T e and n e fluctuations, Astrophysics , 43 , 627-640 (2002) . ...
... We propose the three-phase model for hot star winds and calculate the X-Ray line emission of hot component of wind in a comparison with a XMM-Newton X-Ray spectra of O4f star zeta Puppis. ...
... Emission of the inhomogeneous plasma: line intensities and element abundances in the gaseous nebulae with T e and n e fluctuations , Astrophysics, 43 , 627-640 (2000) . ...
... Emission of the inhomogeneous plasma: line intensities and element abundances in the gaseous nebulae with T e and n e fluctuations , Astrophysics, 43 , 627-640 (2000) . ...
... 1 is not the optimum for creation of hot star discs which, in terms of emission measure for example, is found to occur in a broad peak around So~ 0.5-0.6 depending slightly on the wind velocity law. ...