<--- Back to Details
First PageDocument Content
Black holes / Star types / Accretion disc / Vortices / Binary star / Celestial mechanics / Magnetorotational instability / Monoceros Ring / Accretion / Physics / Astronomy / Space
Date: 2015-02-18 19:22:43
Black holes
Star types
Accretion disc
Vortices
Binary star
Celestial mechanics
Magnetorotational instability
Monoceros Ring
Accretion
Physics
Astronomy
Space

Mon. Not. R. Astron. Soc. 000, 1–[removed]Printed 18 February[removed]MN LATEX style file v2.2)

Add to Reading List

Source URL: users.monash.edu.au

Download Document from Source Website

File Size: 1,50 MB

Share Document on Facebook

Similar Documents

Exciting Waves and Oscillation Modes in Black-Hole Accretion Disks and other Rotating Astrophysical Flows Dong Lai Cornell University

Exciting Waves and Oscillation Modes in Black-Hole Accretion Disks and other Rotating Astrophysical Flows Dong Lai Cornell University

DocID: 1voWK - View Document

POTENTIAL TERM PAPER TOPICS –Feb. 16, 2004 (there could be many more) MOON Analysis of the constraints imposed on lunar and planetary accretion and evolution by the Hf/W isotopic system Analysis of the constraints impo

POTENTIAL TERM PAPER TOPICS –Feb. 16, 2004 (there could be many more) MOON Analysis of the constraints imposed on lunar and planetary accretion and evolution by the Hf/W isotopic system Analysis of the constraints impo

DocID: 1upgj - View Document

THREE-DIMENSIONAL SIMULATIONS OF INSTABILITIES IN ACCRETION DISK TORUS Jung Lin (Doris) Lee ABSTRACT Accretion disks can be found in a variety of astrophysical systems, such as around young stars and black holes. It has

THREE-DIMENSIONAL SIMULATIONS OF INSTABILITIES IN ACCRETION DISK TORUS Jung Lin (Doris) Lee ABSTRACT Accretion disks can be found in a variety of astrophysical systems, such as around young stars and black holes. It has

DocID: 1tLOy - View Document

The emerging paradigm of pebble accretion Chris W. Ormel Abstract Pebble accretion is the mechanism in which small particles (‘pebbles’) accrete onto big bodies (planetesimals or planetary embryos) in gas-rich enviro

The emerging paradigm of pebble accretion Chris W. Ormel Abstract Pebble accretion is the mechanism in which small particles (‘pebbles’) accrete onto big bodies (planetesimals or planetary embryos) in gas-rich enviro

DocID: 1tFWD - View Document