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Fragmentation of Interstellar Clouds
2014The 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.
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Thermal instability in magnetized interstellar clouds
Astronomical & Astrophysical Transactions, 1997Abstract 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
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Translucent Interstellar Clouds
2011A 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.
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Interstellar objects outnumber Solar system objects in the Oort cloud
Monthly Notices of the Royal Astronomical Society: Letters, 2021Amir Siraj, Abraham Loeb, Loeb A
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Observation of interstellar lithium in the low-metallicity Small Magellanic Cloud
Nature, 2012Nicolas Lehner +2 more
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Origin of oort cloud comets in the interstellar space
Celestial Mechanics and Dynamical Astronomy, 1992Seppo Mikkola, Valtonen Mauri J
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Anomalously small magnetic field in the local interstellar cloud
Nature, 1997George Gloeckler +2 more
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The stardust abundance in the local interstellar cloud at the birth of the Solar System
Nature Astronomy, 2017János Kodolányi +2 more
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Interstellar Turbulence II: Implications and Effects
Annual Review of Astronomy and Astrophysics, 2004Bruce Elmegreen, John Scalo
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