Feasibility study of Lense-Thirring precession in LS I +61°303

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Table 1:

Two-peak MQ vs Pulsar Model.
	PSR B1259-63	Two-peak Microquasar	LS I +61 $^{\circ }$ 303
radiopulses	yes	no	no
$L_{\rm X}$ [erg/s]	$5 \times 10^{34}$ ^a	10^33.5-10^36b	$(1{-}6) \times 10^{34}$ ^c
Largest radio outburst	toward periastron^d	toward apastron^e	toward apastron^f
Radio spectral index	$\alpha < 0$ ^d	$\alpha\ge 0$ then $\alpha < 0$ ^g	$\alpha \geq 0$ then $\alpha < 0$ twice per orbit^b
Gamma-ray peak	toward periastron^h	EIC at periastron, dominant SSC toward apastron^e, i	Two peaks: EGRET/VERITAS/FERMIⁱ

Notes. ^(a) Kaspi et al. 1995. ^(b) Massi & Kaufman Bernadó 2009. ^(c) Paredes et al. 1997. ^(d) Connors et al. 2002. ^(e) Bosh-Ramon 2006. ^(f) Fig. 2-c in Massi & Kaufman Bernadó 2009. ^(g) Fender et al. 2004. ^(h) Aharonian et al. 2009. ⁽ⁱ⁾ see Sect. 1.

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