(en) Simon A., Szatmary, K. & Szabo Gy. M., « Determination of the size, mass, and density of exomoons from photometric transit timing variations », Astronomy and Astrophysics, vol. 480, no 2, , p. 727–731 (arXiv0705.1046)
(en) Alex Teachey et David M. Kipping, « Evidence for a large exomoon orbiting Kepler-1625b », Science Advances, vol. 4, no 10, , article no eaav1784 (DOI10.1126/sciadv.aav1784).
(en) René Heller, « Exomoon habitability constrained by energy flux and orbital stability », Astronomy and Astrophysics, vol. 545, , p. L8 (DOI10.1051/0004-6361/201220003, lire en ligne)
(en) René Heller, « Exomoon habitability constrained by energy flux and orbital stability », Astronomy and Astrophysics, vol. 545, , p. L8 (DOI10.1051/0004-6361/201220003, lire en ligne)
iop.org
iopscience.iop.org
(en) Alexandra E. Doyle, Steven J. Desch et Edward D. Young, « Icy Exomoons Evidenced by Spallogenic Nuclides in Polluted White Dwarfs », The Astrophysical Journal Letters, vol. 907, no 2, (lire en ligne).
(ru) Российские астрономы впервые открыли луну возле экзопланеты (en russe) - « Studying of a curve of change of shine of WASP-12b has brought to the Russian astronomers unusual result: regular splashes were found out.<...> Though stains on a star surface also can cause similar changes of shine, observable splashes are very similar on duration, a profile and amplitude that testifies for benefit of exomoon existence. »
sciencedaily.com
(en) [1] - "Mamajek thinks his team could be either observing the late stages of planet formation if the transiting object is a star or brown dwarf, or possibly moon formation if the transiting object is a giant planet"