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NO EVIDENCE OF INTRINSIC OPTICAL/NEAR-INFRARED LINEAR POLARIZATION FOR V404 CYGNI DURING ITS BRIGHT OUTBURST IN 2015: BROADBAND MODELING AND CONSTRAINT ON JET PARAMETERS

  • Authors: Y. T. Tanaka, R. Itoh, M. Uemura, Y. Inoue, C. C. Cheung, M. Watanabe, K. S. Kawabata, Y. Fukazawa, Y. Yatsu, T. Yoshii, Y. Tachibana, T. Fujiwara, Y. Saito, N. Kawai, M. Kimura, K. Isogai, T. Kato, H. Akitaya, M. Kawabata, T. Nakaoka, K. Shiki, K. Takaki, M. Yoshida, M. Imai, S. Gouda, Y. Gouda, H. Akimoto, S. Honda, K. Hosoya, A. Ikebe, K. Morihana, T. Ohshima, Y. Takagi, J. Takahashi, K. Watanabe, D. Kuroda, T. Morokuma, K. Murata, T. Nagayama, D. Nogami, Y. Oasa, and K. Sekiguchi

2016 The Astrophysical Journal 823 35.

  • Provider: AAS Journals

Caption: Figure 2.

R-band PD and PA for V404 Cyg (shown in blue at center) and for surrounding sources (shown in red) within the 7′ × 7′ Kanata/HONIR FOV.

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