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Alan P. Boss
Researcher at Carnegie Institution for Science
Publications - 431
Citations - 40212
Alan P. Boss is an academic researcher from Carnegie Institution for Science. The author has contributed to research in topics: Planet & Formation and evolution of the Solar System. The author has an hindex of 78, co-authored 426 publications receiving 38471 citations. Previous affiliations of Alan P. Boss include Ames Research Center & NASA Headquarters.
Papers
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Book ChapterDOI
Protostars and Protoplanetary Disks
TL;DR: A great wealth of observational information about young stars has been obtained at infrared and longer wavelengths in the last decade, and these observations have pushed our understanding of the overall star formation process to a satisfying level as mentioned in this paper.
Journal ArticleDOI
Formation and Fragmentation of Protostellar and Protoplanetary Disksa
TL;DR: In this article, the authors describe the results of numerical calculations that seek to describe the two-and three-dimensional evolution of nonmagnetic protostellar disks during their formation phases.
Posted Content
Wide-Orbit Exoplanet Demographics
David P. Bennett,Rachel Akeson,Yann Alibert,Jay Anderson,Etienne Bachelet,Jean Phillipe Beaulieu,Jean Phillipe Beaulieu,Andrea Bellini,Aparna Bhattacharya,Aparna Bhattacharya,Alan P. Boss,Valerio Bozza,Stephen T. Bryson,Derek Buzasi,Sebastiano Calchi Novati,Jessie L. Christiansen,Shawn Domagal-Goldman,Michael Endl,Benjamin J. Fulton,Calen B. Henderson,B. Scott Gaudi,Samson A. Johnson,Naoki Koshimoto,Naoki Koshimoto,Naoki Koshimoto,Michael Meyer,Gijs D. Mulders,Susan E. Mullally,Ruth Murray-Clay,David M. Nataf,Eric L. Nielsen,Henry Ngo,Ilaria Pascucci,Matthew T. Penny,Peter Plavchan,Radek Poleski,Clément Ranc,Sean N. Raymond,Leslie A. Rogers,Johannes Sahlmann,Kailash C. Sahu,Joshua E. Schlieder,Yossi Shvartzvald,Alessandro Sozzetti,Rachel Street,Takahiro Sumi,Daisuke Suzuki,Neil Zimmerman +47 more
TL;DR: In this article, the authors summarize current and planned exoplanet detection programs using a variety of methods: microlensing (including WFIRST), radial velocities, Gaia astrometry, and direct imaging.