Figure 2 from Radio Variability of a Fermi Large Area Telescope Bright Source 0FGL J1847.8+3223

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Radio Variability of a Fermi Large Area Telescope Bright Source 0FGL J1847.8+3223

Authors: S. Kida, K. Niinuma, K. Tekefuji, T. Tanaka, T. Aoki, K. Asuma, S. Nakagawa, H. Uehara, H. Akamatsu, A. Imai, H. Miyata, J. Ikouga, A. Otsubo, K. Odai, R. Kodama, Y. Takanashi, N. Nakamizo, Y. Yamada, R. Hiruma, N. Furukawa, N. Matsumura, and T. Daishido

KIDA et al. 2010 The Astrophysical Journal Letters 714 L36.

Provider: AAS Journals

Caption: Figure 2.

Autocorrelation of the fringe surrounded by the red dotted line of Figure 1. All autocorrelations show 41 s that are peculiar periods of an object fixed to the celestial sphere. Left: CGCG 502-027, center: 4C +32.60, and right: B2 1846+32A.

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