The nonthermal radio emission of WR 140 in a model with colliding two-phase winds

Author： Abramova O. Averin P. Bychkov K.

ISSN： 1063-7729

Source： Astronomy Reports, Vol.47, Iss.1, 2003-01, pp. : 31-37

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

Related content

MHD numerical simulations of colliding winds in massive binary systems – I. Thermal versus non-thermal radio emission

By Falceta-Gonçalves D. Abraham Z.

Monthly Notices of the Royal Astronomical Society, Vol. 423, Iss. 2, 2012-06 ,pp. : 1562-1570

Oxford University Press

Access to resources Recommend Favorite

A dissipative model of interacting winds for WR 140: A comparison with observations

By Zhekov S. Myasnikov A.

Astronomy Letters, Vol. 29, Iss. 6, 2003-06 ,pp. : 394-399

MAIK Nauka/Interperiodica

Access to resources Recommend Favorite

Colliding winds in five WR+O systems of the Southern hemisphere

By Fahed R. Moffat A. F. J.

Monthly Notices of the Royal Astronomical Society, Vol. 424, Iss. 3, 2012-08 ,pp. : 1601-1613

Oxford University Press

Access to resources Recommend Favorite

Dust formation in binaries with OB and WR components in a two-phase stellar-wind model

By Aleksandrova O. Bychkov K.

Astronomy Reports, Vol. 45, Iss. 4, 2001-04 ,pp. : 281-286

MAIK Nauka/Interperiodica

Access to resources Recommend Favorite

3D models of radiatively driven colliding winds in massive O + O star binaries – II. Thermal radio to submillimetre emission

By Pittard J. M.

Monthly Notices of the Royal Astronomical Society, Vol. 403, Iss. 4, 2010-04 ,pp. : 1633-1656

Oxford University Press

Access to resources Recommend Favorite