Accretion-Ejection Mechanism of Cygnus X-3(Poster)

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概要

• 論文の詳細を見る

• Cygnus X-3 is one of the brightest sources in radio band among the Galactic microquasars, exhibiting outflows in the form of jets. The X-ray SED shows that the source exists in both low as well as high states, correspondingly related to the radio emission. The X-ray emission shows features unique to this source, independent of its X-ray state as well radio emission. We discuss these properties of this source, as observed, in the recent years, by RXTE.

• 一般社団法人日本物理学会の論文
• 2004-11-15

著者

• Choudhury Manojendu

  Tata Institute Of Fundamental Research

• RAO A.

  Tata Institute of Fundamental Research

関連論文

• Accretion-Ejection Mechanism of Cygnus X-3(Poster)
• Accretion-Ejection Mechanism of Cygnus X-3(Poster)

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