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Fragmentation of Interstellar Clouds

2014
The dense cores that form stars through gravitational collapse are embedded in much larger and more rarefied expanses of gas. How the parent▶molecular cloud produces its substructure of dense cores is the problem of fragmentation. The traditional view is that the parent cloud breaks apart as it collapses in on itself.
openaire   +1 more source

Thermal instability in magnetized interstellar clouds

Astronomical & Astrophysical Transactions, 1997
Abstract The effect of a magnetic field on the ionizational-thermal acoustic instability in the cold diffuse ISM is discussed in this paper. It is found that the frozen-in magnetic field leads to new types of instabilities called “magnetoacoustic” instabilities.
Alexander E. Dudorov   +1 more
openaire   +1 more source

Translucent Interstellar Clouds

2011
A translucent interstellar cloud is one that has visual extinction intermediate between that of a ▶ diffuse cloud and that of a dense ▶molecular cloud. Despite the importance of photochemical processes over much of their extent, translucent clouds contain significant molecular column densities.
openaire   +1 more source

Interstellar objects outnumber Solar system objects in the Oort cloud

Monthly Notices of the Royal Astronomical Society: Letters, 2021
Amir Siraj, Abraham Loeb, Loeb A
exaly  

Observation of interstellar lithium in the low-metallicity Small Magellanic Cloud

Nature, 2012
Nicolas Lehner   +2 more
exaly  

Origin of oort cloud comets in the interstellar space

Celestial Mechanics and Dynamical Astronomy, 1992
Seppo Mikkola, Valtonen Mauri J
exaly  

Anomalously small magnetic field in the local interstellar cloud

Nature, 1997
George Gloeckler   +2 more
exaly  

The stardust abundance in the local interstellar cloud at the birth of the Solar System

Nature Astronomy, 2017
János Kodolányi   +2 more
exaly  

Interstellar Turbulence II: Implications and Effects

Annual Review of Astronomy and Astrophysics, 2004
Bruce Elmegreen, John Scalo
exaly  

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