Author： Shapiro A.I.
Publisher： Springer Publishing Company
ISSN： 0571-7256
Source： Astrophysics, Vol.45, Iss.2, 2002-04, pp. : 215-222
Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.
Abstract
Related content
The Formation of a Cooling Layer in a Partially Optically Thick Shock
Astrophysics and Space Science, Vol. 307, Iss. 1-3, 2007-01 ,pp. :
Access to resources
Recommend
Spectral line formation in a mesoturbulent atmosphere
Astrophysics, Vol. 50, Iss. 2, 2007-04 ,pp. :
Polarized line formation by resonance scattering: Lorentz profile
By Loskutov V.
Astrophysics, Vol. 50, Iss. 2, 2007-04 ,pp. :
Type I migration in optically thick accretion discs
Monthly Notices of the Royal Astronomical Society, Vol. 424, Iss. 4, 2012-08 ,pp. :
Formation and Evolution of Titan’s Atmosphere
Space Science Reviews, Vol. 116, Iss. 1-2, 2005-01 ,pp. :