Photoevaporating transitional discs and molecular cloud cores
Author:
Funder
National Science Foundation of China
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/466/1/1205/10866049/stw3200.pdf
Reference52 articles.
1. Photoevaporation of protoplanetary discs – I. Hydrodynamic models
2. THE 2014 ALMA LONG BASELINE CAMPAIGN: FIRST RESULTS FROM HIGH ANGULAR RESOLUTION OBSERVATIONS TOWARD THE HL TAU REGION
3. Internal structure of a cold dark molecular cloud inferred from the extinction of background starlight
4. THE LONG-TERM EVOLUTION OF PHOTOEVAPORATING PROTOPLANETARY DISKS
5. A powerful local shear instability in weakly magnetized disks. I - Linear analysis. II - Nonlinear evolution
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1. Dust condensation in evolving discs and the composition of planetary building blocks;Monthly Notices of the Royal Astronomical Society;2020-05-04
2. On the Gravitational Instabilities of Protoplanetary Disks;Publications of the Astronomical Society of the Pacific;2019-01-29
3. Evolution of Circumbinary Protoplanetary Disks with Photoevaporative Winds Driven by External Far-ultraviolet Radiation;The Astrophysical Journal;2018-10-29
4. The evolution of the protoplanetary disk with mass influx from a molecular cloud core and the photoevaporation winds;New Astronomy;2018-01
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