Results 131 to 137 of about 264 (137)
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Feedback in galaxy formation with two-phase ISM
2003I present a model for galaxy formation based on the physics of two-phase ISM in pressure equilibrium. In this model gas cools or infalls from an external halo, fragmenting into small clouds. These coagulate to form giant molecular complexes, which collapse and form stars. Supernovae drive superbubbles into the hot phase.
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Detection of 15 NH 2 D in dense cores: a new tool for measuring the 14 N/15 N ratio in the cold ISM
Astronomy and Astrophysics, 2009Núria Marcelino +2 more
exaly
The RWST, a comprehensive statistical description of the non-Gaussian structures in the ISM
Astronomy and Astrophysics, 2019Patrick Hennebelle +2 more
exaly
Dust destruction in the ISM: a re-evaluation of dust lifetimes
Astronomy and Astrophysics, 2011Joseph A Nuth
exaly
Studying the small scale ISM structure with supernovae
Astronomy and Astrophysics, 2010David Branch, N L J Cox
exaly