Observable Signatures of Dust Evolution Mechanisms Which Shape the Planet Forming Regions

Proceedings of the International Astronomical Union - United Kingdom
doi 10.1017/s1743921311020758
Full Text
Abstract

Available in full text

Date
Authors
Publisher

Cambridge University Press (CUP)

Related search

Water in Star- And Planet-Forming Regions

Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences
MathematicsEngineeringAstronomyPhysics
2012English

The Depletion of Water During Dispersal of Planet-Forming Disk Regions

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2017English

Mechanisms by Which Lipids Shape the Reaction Coordinate of GlpG Protease

Biophysical Journal
Biophysics
2018English

Giant Planets Orbiting Metal-Rich Stars Show Signatures of Planet-Planet Interactions

Astrophysical Journal Letters
AstrophysicsAstronomyPlanetary ScienceSpace
2013English

Recent Research for Planet Forming Region

TRENDS IN THE SCIENCES
1998English

Chemical Evolution in High-Mass Star-Forming Regions: Results From the Malt90 Survey

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2013English

Evolution of a Habitable Planet

Annual Review of Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2003English

Signatures of Intergalactic Dust From the First Supernovae

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
1997English

The Mechanisms of RNA SHAPE Chemistry

Journal of the American Chemical Society
BiochemistryColloidCatalysisChemistrySurface Chemistry
2012English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2024 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy