Matteo Cantiello
Affiliations: | 2005-2009 | Utrecht University, Utrecht, Netherlands | |
2010-2011 | Argelander Institute for Astronomy | University of Bonn, Germany, Bonn, Nordrhein-Westfalen, Germany | |
2011-2017 | KITP | University of California, Santa Barbara, Santa Barbara, CA, United States | |
2017- | Center for Computational Astrophysics | Flatiron Institute |
Area:
stellar evolution, binary stars, stellar magnetic fields, thermohaline mixingWebsite:
http://www.matteocantiello.com/Google:
"Matteo Cantiello"
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Publications
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Anders EH, Lecoanet D, Cantiello M, et al. (2023) The photometric variability of massive stars due to gravity waves excited by core convection. Nature Astronomy. 7: 1228-1234 |
Perna R, Lazzati D, Cantiello M. (2021) Electromagnetic Signatures of Relativistic Explosions in the Disks of Active Galactic Nuclei The Astrophysical Journal Letters. 906: L7 |
Dittmann AJ, Cantiello M, Jermyn AS. (2021) Accretion onto Stars in the Disks of Active Galactic Nuclei The Astrophysical Journal. 916: 48 |
Cantiello M, Lecoanet D, Jermyn AS, et al. (2021) On the Origin of Stochastic, Low-Frequency Photometric Variability in Massive Stars The Astrophysical Journal. 915: 112 |
Jermyn AS, Dittmann AJ, Cantiello M, et al. (2021) Stellar Evolution in the Disks of Active Galactic Nuclei Produces Rapidly Rotating Massive Stars The Astrophysical Journal. 914: 105 |
Cantiello M, Jermyn AS, Lin DNC. (2021) Stellar Evolution in AGN Disks The Astrophysical Journal. 910: 94 |
Soares-Furtado M, Cantiello M, MacLeod M, et al. (2021) Lithium Enrichment Signatures of Planetary Engulfment Events in Evolved Stars The Astronomical Journal. 162: 273 |
Khetan N, Izzo L, Branchesi M, et al. (2021) A new measurement of the Hubble constant using Type Ia supernovae calibrated with surface brightness fluctuations Astronomy & Astrophysics. 647: A72 |
Renzo M, Cantiello M, Metzger BD, et al. (2020) The Stellar Merger Scenario for Black Holes in the Pair-instability Gap The Astrophysical Journal Letters. 904: L13 |
Jermyn AS, Cantiello M. (2020) The Origin of the Bimodal Distribution of Magnetic Fields in Early-type Stars The Astrophysical Journal. 900: 113 |