Pier-Emmanuel Tremblay, Ph.D.

Affiliations: 
2011 Université de Montréal, Montréal, Canada 
Area:
Astrophisics
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"Pier-Emmanuel Tremblay"
Mean distance: 3535.3
 

Parents

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Pierre Bergeron grad student 2011 Université de Montréal
 (Analyse spectroscopique d'etoiles naines blanches riches en hydrogene (DA): vers des modeles d'atmosphere ameliores sans parametres libres.)
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Publications

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Caiazzo I, Burdge KB, Tremblay PE, et al. (2023) A rotating white dwarf shows different compositions on its opposite faces. Nature
Cunningham T, Wheatley PJ, Tremblay PE, et al. (2022) A white dwarf accreting planetary material determined from X-ray observations. Nature. 602: 219-222
Zhang Z, Liu MC, Hermes JJ, et al. (2020) COol Companions ON Ultrawide orbiTS (COCONUTS). I. A High-gravity T4 Benchmark around an Old White Dwarf and a Re-examination of the Surface-gravity Dependence of the L/T Transition The Astrophysical Journal. 891: 171
Cunningham T, Tremblay P, Gentile Fusillo NP, et al. (2020) From hydrogen to helium: the spectral evolution of white dwarfs as evidence for convective mixing Monthly Notices of the Royal Astronomical Society. 492: 3540-3552
Veras D, Tremblay P, Hermes JJ, et al. (2020) Constraining planet formation around 6–8 M⊙ stars Monthly Notices of the Royal Astronomical Society. 493: 765-775
Southworth J, Tremblay P, Gänsicke BT, et al. (2020) A white dwarf bound to the transiting planetary system WASP-98 Monthly Notices of the Royal Astronomical Society. 497: 4416-4422
McCleery J, Tremblay P, Fusillo NPG, et al. (2020) $Gaia$ white dwarfs within 40 pc II: the volume-limited northern hemisphere sample Monthly Notices of the Royal Astronomical Society
Marigo P, Cummings JD, Curtis JL, et al. (2020) Carbon star formation as seen through the non-monotonic initial–final mass relation Nature Astronomy. 1-9
Tremblay PE, Fontaine G, Fusillo NPG, et al. (2019) Core crystallization and pile-up in the cooling sequence of evolving white dwarfs. Nature. 565: 202-205
Cummings JD, Kalirai JS, Choi J, et al. (2019) A Novel Approach to Constrain Rotational Mixing and Convective-core Overshoot in Stars Using the Initial–Final Mass Relation The Astrophysical Journal. 871: L18
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