Photoevaporation
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- Arxiv:1801.06185V1 [Astro-Ph.EP] 18 Jan 2018
- Exploring M-Earths with Ultra-Stable Mid-Ir Transit and Phase-Curve Spectroscopy
- Transforming Mini-Neptunes Into Super-Earths in the Habitable Zones of M Dwarfs
- Planet Formation
- Photoevaporation and Disk Dispersal Uma Gorti SETI Institute/NASA Ames Research Center Email: [email protected]
- Cold Giant Planets Evaporated by Hot White Dwarfs
- Photoevaporation Flows in Blister HII Regions: I. Smooth Ionization
- Protoplanetary Disks and Their Evolution
- Rapid Destruction of Protoplanetary Discs Due to External Photoevaporation in Star-Forming Regions
- On the Habitability of Our Universe
- Star Forming Regions in Cepheus
- Viscous Evolution and Photoevaporation of Circumstellar Disks Due to External FUV Radiation Fields
- Disk Dispersal by Star-Driven Photoevaporation Progress and Perspective
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- Photoevaporation of the Jovian Circumplanetary Disk I
- Exoplanet Science Strategy
- Extrasolar Planets: from Dust to New Worlds
- Download This Article in PDF Format