The Formation of a Cooling Layer in a Partially Optically Thick Shock

ISSN： 0004-640X

Source： Astrophysics and Space Science, Vol.307, Iss.1-3, 2007-01, pp. : 121-125

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

Previous Menu Next

Abstract

Related content

Line Formation in a Purely Scattering, Optically Thick Atmosphere

By Shapiro A.I.

Astrophysics, Vol. 45, Iss. 2, 2002-04 ,pp. : 215-222

Springer Publishing Company

Access to resources Recommend Favorite

Type I migration in optically thick accretion discs

By Yamada K. Inaba S.

Monthly Notices of the Royal Astronomical Society, Vol. 424, Iss. 4, 2012-08 ,pp. : 2746-2756

Oxford University Press

Access to resources Recommend Favorite

Cooling of magnetars with internal layer heating

By Kaminker A. Yakovlev D. Potekhin A. Shibazaki N. Shternin P. Gnedin O.

Astrophysics and Space Science, Vol. 308, Iss. 1-4, 2007-04 ,pp. : 423-430

Springer Publishing Company

Access to resources Recommend Favorite

Generation of magnetic fluctuations near a shock front in a partially ionized medium

By Bykov A. Toptygin I.

Astronomy Letters, Vol. 31, Iss. 11, 2005-11 ,pp. : 748-754

MAIK Nauka/Interperiodica

Access to resources Recommend Favorite

Time-dependent behaviour of Lyman α photon transfer in a high-redshift optically thick medium

By Xu Wen Wu Xiang-Ping Fang Li-Zhi

Monthly Notices of the Royal Astronomical Society, Vol. 418, Iss. 2, 2011-12 ,pp. : 853-862

Oxford University Press

Access to resources Recommend Favorite