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2012

2FGL J1311.7-3429 Joins the Black Widow Club

Romani, Roger W.

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We have found an optical/X-ray counterpart candidate for the bright, but presently unidentified, Fermi source 2FGL J1311.7-3429.

This counterpart undergoes large amplitude quasi-sinusoidal optical modulation with a 1.56h (5626s) period.
The modulated flux is blue at peak, with T_eff ~14,000K, and redder at minimum.
Superimposed on this variation are dramatic optical flares.

2FGL J1311.7-3429 Joins the Black Widow Club · Around

Built on

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Similar

Watters, K.P. et al. 2009, ApJ, 695, 1289
2009
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Abdo, A.A. et al. 2010, ApJS, 187, 460
2010
Cited alongside, same era.
Ray, P.S. et al. 2012, Proc. 2011 Fermi Symposium
2011
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Romani, R.W. & Shaw, M.S. 2011, ApJ, 743, L26
2011
Cited alongside, same era.
Abdo, A.A. et al. 2009a, ApJS, 183, 46
Cited in the paper.
Abdo, A.A. et al. 2009b, Science, 325, 840
Cited in the paper.

Then

Takata, J, Wang, & Y. Cheng, K.S. 2011, MNRAS, 415, 1827
2011
Later among the works it cites.
Kong, A. et al. 2012, ApJ, 747, L3
2012
Closest in time.
Nolan, P.L. et al. 2012, ApJS, 199, 31
2012
Closest in time.

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